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  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">OS</journal-id>
<journal-title-group>
<journal-title>Ocean Science</journal-title>
<abbrev-journal-title abbrev-type="publisher">OS</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Ocean Sci.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1812-0792</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/os-11-439-2015</article-id><title-group><article-title>Water level oscillations in Monterey Bay and Harbor</article-title>
      </title-group><?xmltex \runningtitle{Oscillations in Monterey Bay}?><?xmltex \runningauthor{J.~Park et~al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Park</surname><given-names>J.</given-names></name>
          <email>joseph_park@nps.gov</email>
        <ext-link>https://orcid.org/0000-0001-5411-1409</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Sweet</surname><given-names>W. V.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Heitsenrether</surname><given-names>R.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>National Park Service, 950 N. Krome Ave, Homestead, FL, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>NOAA, 1305 East West Hwy, Silver Spring, MD, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>NOAA, 672 Independence Parkway, Chesapeake, VA, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">J. Park (joseph_park@nps.gov)</corresp></author-notes><pub-date><day>8</day><month>June</month><year>2015</year></pub-date>
      
      <volume>11</volume>
      <issue>3</issue>
      <fpage>439</fpage><lpage>453</lpage>
      <history>
        <date date-type="received"><day>13</day><month>October</month><year>2014</year></date>
           <date date-type="rev-request"><day>20</day><month>November</month><year>2014</year></date>
           <date date-type="rev-recd"><day>2</day><month>May</month><year>2015</year></date>
           <date date-type="accepted"><day>12</day><month>May</month><year>2015</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015.html">This article is available from https://os.copernicus.org/articles/11/439/2015/os-11-439-2015.html</self-uri>
<self-uri xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015.pdf">The full text article is available as a PDF file from https://os.copernicus.org/articles/11/439/2015/os-11-439-2015.pdf</self-uri>


      <abstract>
    <p>Seiches  are normal modes of water bodies responding to geophysical
forcings with potential to significantly impact ecology and maritime
operations.  Analysis of high-frequency (1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula>) water level
data in Monterey, California, identifies harbor modes between 10 and
120 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> that are attributed to specific geographic features.
It is found that modal amplitude modulation arises from cross-modal
interaction and that offshore wave energy is a primary driver of these
modes.  Synchronous coupling between modes is observed to
significantly impact dynamic water levels.  At lower frequencies with
periods between 15 and 60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>, modes are independent of
offshore wave energy, yet are continuously present.  This is
unexpected since
seiches normally dissipate after cessation of the driving force,
indicating an unknown forcing.  Spectral and kinematic estimates of
these low-frequency oscillations support the idea that a persistent
anticyclonic mesoscale gyre adjacent to the bay is a potential mode
driver, while discounting other sources.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Bounded physical systems support normal modes.  This is true in
quantum mechanical, astronomical, and terrestrial systems such as
harbors and bays, and owing to the central role that harbors play in
human endeavors, there is a rich history analyzing resonant modes of
bays and harbors (seiches); see, for example, <xref ref-type="bibr" rid="bib1.bibx10" id="text.1"/>, <xref ref-type="bibr" rid="bib1.bibx9" id="text.2"/> and <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx2" id="text.3"/>.</p>
      <p>Monterey Bay, California (Fig. <xref ref-type="fig" rid="Ch1.F1"/>),
is a dynamic and ecologically rich system
influenced by Monterey Submarine Canyon, the California Current,
seasonal upwelling, and inshore countercurrents (California
undercurrent, Davidson current).  Monterey Submarine Canyon is the
prominent bathymetric feature, where tidally coherent internal waves
are nearly an order of magnitude stronger than the open ocean, with the
most intense waves characterized as bores <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx16 bib1.bibx24" id="paren.4"/>, and where hydrodynamic mixing (turbulent kinetic
energy dissipation) reaches 3 orders of magnitude greater than the
open ocean <xref ref-type="bibr" rid="bib1.bibx7" id="paren.5"/>.  Interaction of the regional coastline
and bathymetry with the California Current establishes a persistent
anticyclonic mesoscale vortex adjacent to the bay that is readily
observed in satellite ocean surface temperature images
<xref ref-type="bibr" rid="bib1.bibx29 bib1.bibx26" id="paren.6"/> and in high-resolution hydrodynamic
models <xref ref-type="bibr" rid="bib1.bibx31 bib1.bibx32 bib1.bibx30" id="paren.7"/>.  For example,
Fig. <xref ref-type="fig" rid="Ch1.F2"/> clearly depicts the gyre
expressed in sea surface temperatures from satellite thermal imagery.
Upwelling driven by
local wind forcing interacts with this gyre, resulting in a bifurcated
flow of upwelled water with one branch advected northward near Point
Año Nuevo just north of the bay, and the other directed equatorward
along the outside edge of the bay <xref ref-type="bibr" rid="bib1.bibx26" id="paren.8"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Monterey Bay and Canyon. The location of the wave gauge (CDIP) and
water level gauges are indicated with stars. Station information and
coordinates for the CDIP buoy are provided in <xref ref-type="bibr" rid="bib1.bibx8" id="text.9"/>, and for the
tide gauges in <xref ref-type="bibr" rid="bib1.bibx19" id="text.10"/>. We classify bight modes as having periods
between 2 and 15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> with length scales between 2 and 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>,
and bay modes with periods longer than 15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> and scales from 10 to
40 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>. </p></caption>
        <?xmltex \igopts{width=170.716535pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f01.png"/>

      </fig>

      <p>The bay supports commercial fishing, diving and marine recreation
industries serviced from harbors in Monterey, Moss Landing and Santa
Cruz.  Water level oscillations in the bay and harbors, along with
their associated hydraulic currents, play a significant role in the
safety and operation of these interests, and, from an oceanographic
perspective, <xref ref-type="bibr" rid="bib1.bibx4" id="text.11"/> have posed an open question regarding
the continuous forcing of these modes.  That is, seiches are normally
excited by transient forcings such as seismic or meteorological
events, then tend to lose energy and dissipate; however, modal
oscillations in Monterey Bay are observed to be continuously present.
Furthermore, <xref ref-type="bibr" rid="bib1.bibx5" id="text.12"/> noted that
“it is difficult to conceive that such oscillations occur only in
Monterey Bay, and, if it turns out that the excitation is global in
nature, then our results may apply to other resonant basins around
the world as well”.  We therefore have two open research questions
before us: what is the origin of these continuous modes, and, are
they peculiar to Monterey Bay?</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Sea surface temperature image from 13 October 2008 depicting the
persistent mesoscale anti-cyclonic gyre offshore of Monterey Bay. Image from
<xref ref-type="bibr" rid="bib1.bibx28" id="text.13"/>. </p></caption>
        <?xmltex \igopts{width=170.716535pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f02.png"/>

      </fig>

      <p>The seminal study of bay modes was contributed by <xref ref-type="bibr" rid="bib1.bibx35" id="text.14"/>,
who applied analytical and numerical models of increasing
sophistication to characterize the oscillations.  While some of the
numerical results were unsatisfying, the breadth and depth of the
analysis were pioneering, and many of the fundamental results
quantifying bay modes have been corroborated over ensuing decades.
Wilson et al. (1965) assumed that “the surge phenomenon in Monterey Harbor
is the consequence of surf-beats or of genuine long-period waves”,
concluding that the latter was likely the cause, and it is notable
that previous studies did indicate the continuous presence of
oscillations.  For example, <xref ref-type="bibr" rid="bib1.bibx11" id="text.15"/> analyzed a 6-month
wave gauge record and found that 8–22 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> period waves were
present nearly 100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of the time, and <xref ref-type="bibr" rid="bib1.bibx25" id="text.16"/>
examined a 3-year tide gauge record, finding that “shorter waves
(1.5–2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>) are recorded almost continuously”; however, we
believe that <xref ref-type="bibr" rid="bib1.bibx4" id="text.17"/> were the first to conclusively
observe that long-period bay-wide oscillations are effectively
stationary and to question their genesis.</p>
      <p><?xmltex \hack{\newpage}?><xref ref-type="bibr" rid="bib1.bibx5" id="text.18"/> contributed a comprehensive review and analysis of
Monterey Bay oscillations, and based on measurements over an 18 month
period determined primary bay modes at the Monterey tide gauge of
55.9, 36.7, 27.4, 21.8, 18.4 and 16.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>, broadly consistent
with the work of Wilson et al. (1965). There is general agreement that the
55.9 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> mode represents the fundamental longitudinal mode
(north–south), while the 36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> harmonic is attributed to
the primary transverse mode (east–west; refer to
<xref ref-type="fig" rid="Ch1.F1"/>).  It is also accepted that
Monterey Submarine Canyon acts to decouple the bay into two
weakly coupled oscillators, one north of the canyon and one south.
Regarding Monterey Harbor, estimates of modal periods are more
variable, with most sources suggesting periods of 1–2 to
13.3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>, and several making specific mention of
9–10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>.</p>
      <p>Previous observational studies (reviewed in <xref ref-type="bibr" rid="bib1.bibx5" id="altparen.19"/>) used
water level data sampled at (or averaged to) daily, hourly, 6, 4
or 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> intervals such that periods below several minutes are
not resolved.  Here, we examine a 63 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">day</mml:mi></mml:math></inline-formula> record of
1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> water level recorded at the National Oceanic and
Atmospheric Administration (NOAA) Monterey tide gauge allowing
spectral characterization of water level variance to periods as short
as 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>, which to our knowledge is the highest-resolution analysis
of modal oscillations in the bay.  This high-resolution data are used
to quantify and
attribute water level oscillation modes in Monterey Bay and Harbor
to physical processes and boundary conditions.  We also analyze
a 17.8 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">year</mml:mi></mml:math></inline-formula> record of 6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> water levels to characterize
modes associated with bay-wide resonances, which to our knowledge is
the longest continuous record of water levels analyzed for modal
oscillations in the bay.  This novel combination of data allows
us to examine potential mode drivers of both harbor and bay-wide
oscillations, clarifying the roles of potential mode drivers
suggested by <xref ref-type="bibr" rid="bib1.bibx5" id="text.20"/> and suggesting a new one.</p>
</sec>
<sec id="Ch1.S2">
  <title>Length scales</title>
      <p>The dispersion relation for surface gravity waves dictates length
scales corresponding to water depth and oscillation period (resolved
from spectral analysis), and we characterize water level oscillations
as belonging to bay, bight or harbor modes according to spatial scales
appropriate to each domain as shown in Table <xref ref-type="table" rid="Ch1.T1"/>.  We define
harbor oscillations as modes with periods less than 180 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> and
wavelengths less than 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> matching spatial scales within the
breakwater of Monterey Harbor
(Figs. <xref ref-type="fig" rid="Ch1.F1"/> and
<xref ref-type="fig" rid="Ch1.F5"/>).  Modes with periods between 2 and
15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> and length scales between 2 and 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> are
considered bight modes associated with resonances between Point Pinos
at the tip of Monterey Peninsula and the eastern shore of the bay.
Bay modes have periods longer than 15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> and scales from 10
to 40 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>.  The lowest-frequency bay modes correspond to the
longitudinal and transverse lengths of the bay.</p>
</sec>
<sec id="Ch1.S3">
  <title>Observations</title>
      <p>Observations consist of a 63 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">day</mml:mi></mml:math></inline-formula> record (14 September through
29 November 2013) of 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> water level from a microwave ranging
sensor at the NOAA tide station located on Monterey Municipal
Wharf no. 2, a 17.8 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">year</mml:mi></mml:math></inline-formula> record of
6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> water levels (23 August 1996–30 June 2014) from an
acoustic ranging tide gauge located 4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> shoreward of the
microwave sensor, and offshore wave height estimated every
30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> over the 63 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">day</mml:mi></mml:math></inline-formula> record of 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> data
from the Coastal Data Information Program (CDIP) buoy
located approximately 15.2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> WSW of Moss Landing above
Monterey Submarine Canyon.  Station information and
coordinates for the CDIP buoy are provided in <xref ref-type="bibr" rid="bib1.bibx8" id="text.21"/>,
and for the tide gauges in <xref ref-type="bibr" rid="bib1.bibx19" id="text.22"/>.  Gauge
locations are shown in Fig. <xref ref-type="fig" rid="Ch1.F1"/>
with the white stars.</p>
      <p>Since the bay and harbor oscillations are at much higher frequencies
than the tides, we remove the tidal signal from the 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> water
level and analyze the water level nontide residual (NTR).  The tidal
response is obtained from standard NOAA tidal predictions at the
Monterey tide gauge derived from 37 harmonic constituents over the
tidal datum epoch of 1983 to 2001 <xref ref-type="bibr" rid="bib1.bibx20" id="paren.23"/>.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><caption><p>Spatial scales of the bay, bight and harbor modes according to the
dispersion relation <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mi>g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>k</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mtext>tanh</mml:mtext><mml:mo>(</mml:mo><mml:mi>k</mml:mi><mml:mi>d</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> where <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula> is
frequency, <inline-formula><mml:math display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> the wave number, <inline-formula><mml:math display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> the water depth and <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> the
wavelength. The bay and bight modes use depths of 60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>, the harbor
modes 7.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="6">
     <oasis:colspec colnum="1" colname="col1" align="right"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry namest="col1" nameend="col2" align="center">Bay </oasis:entry>  
         <oasis:entry namest="col3" nameend="col4" align="center">Bight </oasis:entry>  
         <oasis:entry namest="col5" nameend="col6" align="center">Harbor </oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Period</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Period</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">Period</oasis:entry>  
         <oasis:entry colname="col6"><inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">(min)</oasis:entry>  
         <oasis:entry colname="col2">(km)</oasis:entry>  
         <oasis:entry colname="col3">(min)</oasis:entry>  
         <oasis:entry colname="col4">(km)</oasis:entry>  
         <oasis:entry colname="col5">(s)</oasis:entry>  
         <oasis:entry colname="col6">(m)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">55.9</oasis:entry>  
         <oasis:entry colname="col2">40.7</oasis:entry>  
         <oasis:entry colname="col3">10.1</oasis:entry>  
         <oasis:entry colname="col4">7.4</oasis:entry>  
         <oasis:entry colname="col5">112</oasis:entry>  
         <oasis:entry colname="col6">480</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">36.7</oasis:entry>  
         <oasis:entry colname="col2">26.7</oasis:entry>  
         <oasis:entry colname="col3">9.0</oasis:entry>  
         <oasis:entry colname="col4">6.5</oasis:entry>  
         <oasis:entry colname="col5">60</oasis:entry>  
         <oasis:entry colname="col6">252</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">27.4</oasis:entry>  
         <oasis:entry colname="col2">19.9</oasis:entry>  
         <oasis:entry colname="col3">4.2</oasis:entry>  
         <oasis:entry colname="col4">3.1</oasis:entry>  
         <oasis:entry colname="col5">41</oasis:entry>  
         <oasis:entry colname="col6">172</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">21.7</oasis:entry>  
         <oasis:entry colname="col2">15.8</oasis:entry>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">31</oasis:entry>  
         <oasis:entry colname="col6">133</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">18.4</oasis:entry>  
         <oasis:entry colname="col2">13.4</oasis:entry>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">16</oasis:entry>  
         <oasis:entry colname="col6">67</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">16.5</oasis:entry>  
         <oasis:entry colname="col2">12.0</oasis:entry>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">12</oasis:entry>  
         <oasis:entry colname="col6">50</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p>Significant wave height (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) at the Monterey Canyon CDIP buoy
(30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> data) and 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> nontide residual water (NTR) levels
from the NOAA tide gauge in Monterey Harbor.
</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f03.png"/>

      </fig>

      <p>Continuous availability of the 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> data was not achieved,
resulting in five segments of lengths 12.1, 12.3, 14.3, 10.5 and
14.1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">days</mml:mi></mml:math></inline-formula> as shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/> exhibiting
a relationship between nontide residual and offshore wave height.
The magnitude of nontide residual is observed to be strongly correlated
with wave height, and should be related to the canonical
definition of significant wave height <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula>,
where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the zeroth moment of the water elevation
spectrum and <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> the standard deviation of water level.
However, here, the water level variance and the significant wave height
are not collocated, and it is known that non-wave-driven processes
such as wind-driven setup and local oscillations also contribute to
the variance such that the canonical relationship is not expected
to be realized.  Nonetheless, it is worth noting that water level
variance estimates from tide gauges are robustly related to wave
height and do have potential as proxies of wave height estimates
<xref ref-type="bibr" rid="bib1.bibx22 bib1.bibx14 bib1.bibx21" id="paren.24"/>.</p>
</sec>
<sec id="Ch1.S4">
  <title>Oscillations in Monterey Harbor</title>
      <p>Figure <xref ref-type="fig" rid="Ch1.F4"/> presents 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> water
level data over 14 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">days</mml:mi></mml:math></inline-formula> of November 2013, the corresponding
spectrogram of a 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> nontide residual computed with
60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> windows and 50 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> overlap, and a power spectral
density (PSD) estimate of the 14 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">day</mml:mi></mml:math></inline-formula>, 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> nontide
residual.  Power spectral densities are estimated by periodogram with
a split cosine bell taper and modified Daniell smoother
<xref ref-type="bibr" rid="bib1.bibx3" id="paren.25"/>.  The PSD indicates that dominant harbor energy
is found at periods of 112, 60, 41, 31, 16 and 12 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>, and are
marked with vertical dashed lines.  Bight modes are also identified
with dash-dot lines (10.1, 9.0 and 4.2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>), and bay modes
with dashed lines (55.9, 36.7, 27.4, 21.8, 18.4 and 16.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>).
Bight and bay modes are discussed in a following section.</p>
<sec id="Ch1.S4.SS1">
  <title>Harbor modes</title>
      <p>Harbor modes are typified by smooth broad peaks in the PSD, suggesting
that for a specific harbor component, there are multiple harmonic
oscillators closely grouped in wave-number space, leading us to expect
that there will be a nearly continuous range of spatial scales
contributing to these modes.  In addition to the broad spectral peak
centered on 112 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>, there are also distinct spectral lines near
112 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> indicating specific resonant scales.  The spectrogram
reveals a time-dependent intensity of harbor modes, for example, the
generally low amplitudes around 25 November and high amplitudes
following 27 November.  Referring to Fig. <xref ref-type="fig" rid="Ch1.F3"/>
suggests that offshore wave height influences harbor amplitudes.
Another interesting feature is the frequency modulation (FM) of modes
coherent with the tidal signal.  We believe that this frequency
modulation arises from the changing water depth and shoreline profile
as mean water level rises and falls such that different length scales
for surface waves are realized.  These spectral features are
representative of all 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> data.</p>
      <p>Figure <xref ref-type="fig" rid="Ch1.F5"/> shows a chart of the harbor
with colored arrows corresponding to resonant mode length scales
governed by the dispersion relation at a water depth of 7.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>
from mode periods identified in Fig. <xref ref-type="fig" rid="Ch1.F4"/>.
The highest-frequency modes with periods less than 30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> are
not depicted in Fig. <xref ref-type="fig" rid="Ch1.F5"/>; they are
associated with reflections from wharf infrastructure.
It should be noted that standing waves form nodes at multiples
of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> from a reflective fixed boundary, and at multiples of
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> from an open boundary so that the lowest-frequency
standing wave (mode) between two reflectors corresponds to a
distance of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>, and in the case of a mode between an
open boundary such as the tide gauge on the wharf and a reflector,
a distance of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula>. Given this, we attribute the
30 and 60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> modes to reflections from the
breakwater protecting the mooring docks, the 41 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>
mode to a standing wave within the mooring docks, and
the dominant harbor mode near 112 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> to
reflections between the inner and outer breakwaters.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <title>Wave height</title>
      <p>To assess the wave dependence of harbor mode amplitudes,
Fig. <xref ref-type="fig" rid="Ch1.F6"/> presents NTR PSD estimates during
three 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> periods when offshore wave height was increasing.
With a significant wave height of 0.8 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> (dominant period
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>5.9</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>), the characteristic harbor modes are
broadly observed with the 60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> period reflection from the
breakwater well resolved.  As significant wave height grows from 0.8
to 1.1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>, most of the energy increase is contained in the band
between 80 and 300 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>, suggesting that it is a combination of
growing reflections from the rocky shore to the west, the breakwater
to the north and a bight mode contributing to increased NTR variance.
When offshore wave height reaches 2.4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>12.5</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>), there is a significant increase in
energy at all modes, and a conspicuous broadening of the 80 to
120 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> resonances suggesting that a rich set of closely spaced
modes is being driven.  We also note that spectral shapes are
essentially invariant as offshore waves transition from periods of 6
to 12 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> but the amplitudes increase, indicating that these
modes are generated by local resonances in the harbor forced by
offshore wave energy, but independent of wave period.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p><bold>(a)</bold> Raw 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> water levels from 15 November 2013
through 29 November 2013. <bold>(b)</bold> Spectrogram of the water levels.
<bold>(c)</bold> Power spectral density estimates of nontide residual water
levels. Dashed vertical lines mark the bay-wide resonance modes (55.9, 36.7,
27.4, 21.8, 18.5 and 16.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>), dash-dot lines mark bight periods
(10.1, 9.0 and 4.2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>) and dotted lines the harbor modes (112, 60,
41, 31, 16 and 12 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>). </p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f04.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p>Chart of Monterey Harbor with resonant mode length scales corresponding to
periods observed in the power spectra. The tide gauge location is denoted by
the star. Wavelengths are determined from the general dispersion relation
applied at a depth of 7.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>. Spatial scales of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> are
sustained between two reflective boundaries, while the fundamental length of
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> corresponds to one open boundary such as the tide gauge on the
wharf and one reflective boundary. Chart is number 18 685 from the NOAA
National Ocean Service Coast Survey.
</p></caption>
          <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f05.png"/>

        </fig>

      <p>To quantify the amplitude dependence of offshore wave height on harbor
and bay oscillations, we regress PSD amplitudes of the dominant harbor
and bay modes (112 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> and 36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>, respectively)
against offshore significant wave height (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>):

                <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>PSD</mml:mtext><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msubsup><mml:mi>H</mml:mi><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>PSD</mml:mtext><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> NTR PSD amplitudes in
dB of the 36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> or 112 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> modes over a 24 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula>
sliding window advanced in 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> increments over all data.
Figure <xref ref-type="fig" rid="Ch1.F7"/> plots the data and model fits,
indicating that the harbor mode responds to offshore wave amplitude
with nonlinear growth (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn>0.70</mml:mn></mml:mrow></mml:math></inline-formula>), while the bay mode has no such
dependence (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mn>0.03</mml:mn></mml:math></inline-formula>).</p>
</sec>
<sec id="Ch1.S4.SS3">
  <title>Wave direction</title>
      <p>To examine offshore wave direction in the forcing of harbor modes,
Fig. <xref ref-type="fig" rid="Ch1.F8"/>a plots NTR PSD estimates from two
periods when offshore significant wave heights were small
(0.5–0.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>), and the dominant wave direction was either west
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn>250</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> N) or northwest (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn>295</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> N).  With the
exception of the 15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> resonance, harbor modes are
significantly enhanced when low-amplitude waves are arriving from the
northwest instead of the west.  This is consistent with the wave
refraction analysis presented by <xref ref-type="bibr" rid="bib1.bibx35" id="text.26"/> indicating that
wave energy from the west is less efficiently refracted into the
harbor than waves from the northwest.</p>
      <p>Figure <xref ref-type="fig" rid="Ch1.F8"/>b presents NTR PSD estimates
from larger waves and arrival directions of west
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn>265</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> N) and northwest (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn>297</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> N). Here,
a comparison of the NTR spectra finds that wave direction has a smaller
influence on harbor mode amplitudes then when waves are small,
although some specific modes such as those with 9 and 60 s
periods are enhanced.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S4.SS4">
  <title>Tidal phase</title>
      <p>Spectrograms of 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> data indicate that tidal phase serves to
modulate the frequency of harbor modes as shown in Fig. <xref ref-type="fig" rid="Ch1.F4"/>b. To examine this, we selected
a period with minimum offshore wave height covering a semidiurnal
tidal cycle (25 November, 04:30 to 14:00 UTC).  This cycle
corresponds to the largest
semidiurnal cycle of the day with a range of roughly 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>, which
is close to the mean tidal range of 1.08 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>. The water depth at
the sensor is nominally 9.1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> at MLLW, so that the water depth
to mean tidal range ratio is roughly 9 to 1.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p>Power spectral density estimates of 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> nontide residual
over 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> periods during 20 and 21 September 2013 with different deep
water wave heights. Dotted vertical lines mark the harbor modes at 112, 60,
41, 31, 16 and 12 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>. </p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><caption><p><bold>(a)</bold> Water level amplitudes at the dominant harbor period of
112 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>, and <bold>(b)</bold> amplitudes at the dominant bay period
of 36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> as a function of significant wave height.  Each
amplitude is estimated from a PSD computed over an 18 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> moving
window with a time increment of 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula>.  Solid lines are a least
squares fit to a nonlinear model (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mtext>PSD</mml:mtext><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msubsup><mml:mi>H</mml:mi><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>).
Note that the water level amplitudes are in dB.
</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f07.png"/>

        </fig>

      <p>To compare the spectral response of these two tidal regimes, we
computed NTR PSD
estimates over 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> periods centered on the low (04:30–06:30)
and high water (12:00–14:00) tidal phases as shown in
Fig. <xref ref-type="fig" rid="Ch1.F9"/>.  There is a clear shift from
longer to shorter periods at high water in relation to low water,
supporting the idea that water depth and associated shoreline
boundary condition characteristics influence the modal structure
of the harbor.</p>
      <p>We note that this
cycle was during a neap tide, and expect that, during spring tide, the
tidal dependence on harbor oscillation frequencies will be even more
pronounced.  For example, in Fig. <xref ref-type="fig" rid="Ch1.F4"/>b,
we noted the frequency
modulation of harbor modes with tidal phase where the tidal range
exceeded 2 m, and one can clearly see the changing frequencies of
the harbor modes.</p>
</sec>
<sec id="Ch1.S4.SS5">
  <title>Dynamic mode response</title>
      <p>The dynamic characteristics of harbor modes can be assessed by
decomposing the 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> nontide residuals into components
capturing temporal variations at different timescales with a maximal
overlap discrete wavelet transform (MODWT, <xref ref-type="bibr" rid="bib1.bibx23" id="altparen.27"/>).  The
MODWT is defined in Appendix A and we employ an 11-level
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>J</mml:mi><mml:mo>=</mml:mo><mml:mn>11</mml:mn></mml:mrow></mml:math></inline-formula>) transform based on the least asymmetric mother
wavelet (LA8).  Approximate temporal scales for the wavelet levels are
listed in Table <xref ref-type="table" rid="Ch1.T2"/>.</p>
      <p>Figure <xref ref-type="fig" rid="Ch1.F10"/> plots the MODWT decomposition for two of the
2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> periods shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/>.  The
bottom panel of each plot shows the NTR time series with panels above
in ascending order plotting the wavelet coefficients for each level of
increasing timescale. The wavelet coefficients of each level are scaled
by their respective magnitude squared so that the amplitude
represents the partial variance contributed by each level.  With
offshore significant wave heights of
0.8 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> (0–2000 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> in Fig. <xref ref-type="fig" rid="Ch1.F10"/>a), the NTR
energy is fairly evenly distributed between the W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>,
W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>, W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>, W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>10</mml:mn></mml:msub></mml:math></inline-formula> and W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>11</mml:mn></mml:msub></mml:math></inline-formula> levels corresponding to temporal
scales of 15, 31, 59, 99, 900 and 1800 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>.  As waves grow from
0.8 to 1.1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> (3000–7000 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> in Fig. <xref ref-type="fig" rid="Ch1.F10"/>a),
the W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula> levels exhibit the emergence of
oscillatory modes at timescales of 96 and 126 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>, consistent
with the spectral perspective shown in
Fig. <xref ref-type="fig" rid="Ch1.F6"/>.  When waves have grown to
2.4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>, we find in Fig. <xref ref-type="fig" rid="Ch1.F10"/>b that the
W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>, W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula> timescales (58, 101,
117 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>) dominate the NTR energy, again consistent with
the Fourier decomposition in Fig. <xref ref-type="fig" rid="Ch1.F6"/>.  The
same general behavior with the emergence, growth and dominance of the
50 to 120 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> modes in Monterey Harbor during wave events is
robustly observed.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2"><caption><p>Wavelet level dominant periods in seconds.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.95}[.95]?><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1">Level</oasis:entry>  
         <oasis:entry colname="col2">9/20 22:00–</oasis:entry>  
         <oasis:entry colname="col3">9/21 16:00–</oasis:entry>  
         <oasis:entry colname="col4">10/4 10:00–</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">–24:00 UTC</oasis:entry>  
         <oasis:entry colname="col3">–18:00 UTC</oasis:entry>  
         <oasis:entry colname="col4">–12:00 UTC</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 0.8–1.1 (m)</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 2.4 (m)</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 2.0 (m)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">W2</oasis:entry>  
         <oasis:entry colname="col2">13</oasis:entry>  
         <oasis:entry colname="col3">12</oasis:entry>  
         <oasis:entry colname="col4">9</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">W3</oasis:entry>  
         <oasis:entry colname="col2">15</oasis:entry>  
         <oasis:entry colname="col3">14</oasis:entry>  
         <oasis:entry colname="col4">12</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">W4</oasis:entry>  
         <oasis:entry colname="col2">31</oasis:entry>  
         <oasis:entry colname="col3">31</oasis:entry>  
         <oasis:entry colname="col4">30</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">W5</oasis:entry>  
         <oasis:entry colname="col2">60</oasis:entry>  
         <oasis:entry colname="col3">58</oasis:entry>  
         <oasis:entry colname="col4">61</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">W6</oasis:entry>  
         <oasis:entry colname="col2">96</oasis:entry>  
         <oasis:entry colname="col3">101</oasis:entry>  
         <oasis:entry colname="col4">111</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">W7</oasis:entry>  
         <oasis:entry colname="col2">126</oasis:entry>  
         <oasis:entry colname="col3">117</oasis:entry>  
         <oasis:entry colname="col4">118</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">W8</oasis:entry>  
         <oasis:entry colname="col2">486</oasis:entry>  
         <oasis:entry colname="col3">405</oasis:entry>  
         <oasis:entry colname="col4">260</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">W9</oasis:entry>  
         <oasis:entry colname="col2">729</oasis:entry>  
         <oasis:entry colname="col3">663</oasis:entry>  
         <oasis:entry colname="col4">911</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">W10</oasis:entry>  
         <oasis:entry colname="col2">800</oasis:entry>  
         <oasis:entry colname="col3">830</oasis:entry>  
         <oasis:entry colname="col4">800</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">W11</oasis:entry>  
         <oasis:entry colname="col2">1030</oasis:entry>  
         <oasis:entry colname="col3">1090</oasis:entry>  
         <oasis:entry colname="col4">1285</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <p>An interesting feature of these primary harbor modes (W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>,
W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula>) is their temporal amplitude modulation (AM).
These AM effects are generally not synchronous across levels, and
appear to have modulation periods in the neighborhood of
20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>.  These periods are not representative of the bay or
bight modes previously identified, and  their non-synchronous nature
suggests that they are not forced by a unitary driver, e.g., long-period waves propagating from offshore.  However, we previously noted
the broad spectral nature of the harbor modes indicative of multiple
harmonic oscillators closely spaced in frequency/wave number, and this
leads us to speculate that the AM arises from superposition of closely
spaced modes in frequency space.  To test this hypothesis, we select 10
spectral amplitudes from the NTR PSD with 2.4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> wave height
from Fig. <xref ref-type="fig" rid="Ch1.F6"/> at periods of 58, 83, 94, 97,
100, 104, 107, 112 116 and 209 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>, and create a reconstruction
from these components with a harmonic superposition:

                <disp-formula id="Ch1.E2" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mi>i</mml:mi></mml:munder><mml:msub><mml:mi>A</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi>sin⁡</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the NTR spectral amplitude and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> the frequency.  This reconstruction is compared
to the W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> level in Fig. <xref ref-type="fig" rid="Ch1.F11"/>
where the envelope has been plotted for each time series.
Qualitatively, the overall AM behavior of the reconstructed
superposition and the actual mode is similar, leading to the
suggestion that it is cross-modal interference of closely spaced
harbor modes resulting in the AM of specific resonances.  Although the
AM envelopes are generally not synchronous, there is nothing
precluding them from randomly aligning, and in
Fig. <xref ref-type="fig" rid="Ch1.F12"/> we present evidence of such
an alignment between the W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula> levels
suggesting that when modes synchronize, their impact on the overall NTR
can be significant.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3"><caption><p>Mean water level spectral amplitudes at the bay-wide oscillation
modes estimated from 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> nontide residuals over 63 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">days</mml:mi></mml:math></inline-formula>. The
95 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> confidence interval on spectral amplitude is 3.0 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">dB</mml:mi></mml:math></inline-formula>.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="right"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1">Period</oasis:entry>  
         <oasis:entry colname="col2">PSD dB</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>dB</oasis:entry>  
         <oasis:entry colname="col4">Water level</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">(min)</oasis:entry>  
         <oasis:entry colname="col2">(<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Hz</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col3">(<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Hz</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col4">(m)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">36.7</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>9.3</oasis:entry>  
         <oasis:entry colname="col3">0.0</oasis:entry>  
         <oasis:entry colname="col4">0.341</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">27.4</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>12.8</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.4</oasis:entry>  
         <oasis:entry colname="col4">0.230</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">55.9</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13.3</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.0</oasis:entry>  
         <oasis:entry colname="col4">0.215</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">21.7</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15.7</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6.4</oasis:entry>  
         <oasis:entry colname="col4">0.164</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">18.4</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>17.8</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8.4</oasis:entry>  
         <oasis:entry colname="col4">0.129</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">16.5</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>17.9</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8.5</oasis:entry>  
         <oasis:entry colname="col4">0.128</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
</sec>
<sec id="Ch1.S5">
  <title>Oscillations in Monterey Bay</title>
      <p>The bay modes are clearly identified in 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> spectra
(Fig. <xref ref-type="fig" rid="Ch1.F4"/>) and we estimate their water
level amplitudes over the 63 day period by computing mean PSD
amplitudes over all 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> data over a sliding window of
24 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> advanced in 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> increments.  The modes are ranked
in terms of decreasing amplitude in Table <xref ref-type="table" rid="Ch1.T3"/> indicating that the
36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> mode exhibits the highest average power.  Improved
spectral resolution is afforded by a longer record and
Fig. <xref ref-type="fig" rid="Ch1.F13"/> presents a spectrogram
and PSD of a 17.8 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">year</mml:mi></mml:math></inline-formula> record of 6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> water level data.
Spectrogram PSDs are from records of 2048 points (8.53 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">days</mml:mi></mml:math></inline-formula>)
with 50 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> overlap.  The two dominant features are the annual
occurrence of increased broadband variance from winter storms
(vertical bands), and the continuously present energy at the bay
periods quantified by <xref ref-type="bibr" rid="bib1.bibx5" id="text.28"/>.</p>
      <p>The PSD reveals that the 36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> transverse bay mode (east–west)
is not only the most energetic, but is actually also a series of closely spaced
modes.  The 27.4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>
mode exhibits a high quality (<inline-formula><mml:math display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula>) factor (ratio of energy stored in
the mode resonance to energy supplied driving the resonance) as
evidenced by the high signal-to-noise ratio and narrow
bandwidth of the spectral peak indicating a resonance highly tuned to
the source.  According to <xref ref-type="bibr" rid="bib1.bibx5" id="text.29"/> and <xref ref-type="bibr" rid="bib1.bibx35" id="text.30"/>
the spatial harmonics of this mode correspond to partitioning of the
bay into thirds with northern, central (canyon) and southern
regions, which would suggest that this mode is efficiently tuned to
the decoupling of the southern and northern parts of the bay by the canyon,
whereas the fundamental longitudinal mode (55.9 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>) is not.
It is not clear why this would be the case.  The dominance of these
modes suggests that they are the modes most directly coupled to the
unknown continuous forcing of bay oscillations.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><caption><p><bold>(a)</bold> Power spectral density estimates of 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula>
nontide residual water level over 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> periods with offshore
significant wave heights of 0.5 and 0.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> and arrival directions of
250 and 295<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. <bold>(b)</bold> Power spectral density estimates of
1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> nontide residual water level over 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> periods with
offshore significant wave heights of 2.0 and 2.1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> and arrival
directions of 265 and 297<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. Dotted lines correspond to harbor
modes (112, 60, 41, 31, 16 and 9 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>).
</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f08.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><caption><p>PSD estimates of 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> NTR data from 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> periods
centered on low and high water of a tidal period. Offshore waves were low
during this period. Dotted vertical lines mark harbor modes at 112, 60, 41,
31, 16 and 12 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>. </p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f09.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p><bold>(a)</bold> Discrete wavelet transform decomposition of nontide residual
during a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> period when deep water significant wave height increased
from 0.8 to 1.1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>. The red box highlights the W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula> wavelet
levels exhibiting emergence of energy in these two bands as wave height
increases. <bold>(b)</bold> Discrete wavelet transform decomposition of nontide
residual during a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> period when deep water significant wave height
was 2.4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>. The red box highlights the W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>, W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula> wavelet
levels exhibiting dominance of energy in these bands and amplitude
modulation. Power spectral density estimates of these 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> period are
shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/>.
</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f10.png"/>

      </fig>

<sec id="Ch1.S5.SS1">
  <title>Mode forcing</title>
      <p><xref ref-type="bibr" rid="bib1.bibx5" id="text.31"/> considered six physical mechanisms as prospective
forcings for continuous oscillations of the bay:
<list list-type="order"><list-item>
      <p>edge waves,</p></list-item><list-item>
      <p>long-period surface waves,</p></list-item><list-item>
      <p>sea breeze,</p></list-item><list-item>
      <p>internal waves,</p></list-item><list-item>
      <p>microseisms, and</p></list-item><list-item>
      <p>small-scale turbulence,</p></list-item></list>
and noted that the first three are not likely to be continuously present,
and so are not consistent with the observation of persistent
oscillations.  Tidally synchronous internal waves have been observed
propagating up the submarine canyon and episodically transitioning to
bores <xref ref-type="bibr" rid="bib1.bibx16 bib1.bibx18 bib1.bibx7" id="paren.32"/>; their tidal coupling
suggests a continuous presence and potential mode forcing.
Microseisms are an appealing candidate due to their omnipresence
<xref ref-type="bibr" rid="bib1.bibx15" id="paren.33"/>; however, it was speculated that their energy was
insufficient at the bay frequencies to drive the oscillations.
Breaker et al. (2010) also discounted small-scale turbulence on the basis of
its intermittent nature.  These arguments are based primarily on
temporal persistence; however, we offer an alternative perspective
based on kinematic energy scales.</p>
      <p><?xmltex \hack{\newpage}?>Under the assumption that the 36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> mode is the directly
forced fundamental mode, we can ask questions regarding its observed
amplitude and spectral resonance to grossly estimate the energy
required to sustain it.  Table <xref ref-type="table" rid="Ch1.T3"/> indicates that the rms (root mean square) water
level deviation of this mode at the Monterey tide gauge is
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>h</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>0.341</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>.  Neglecting the effect of
shoaling on wavelength, a raised-cosine profile with <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>=</mml:mo><mml:mn>26.7</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> (Table <xref ref-type="table" rid="Ch1.T1"/>) approximates the cross-shore
elevation of the mode, with a profile area of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>9104</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>.  <xref ref-type="bibr" rid="bib1.bibx5" id="text.34"/> assessed spatial harmonics
of bay modes with a regional ocean modeling system (ROMS)
implementation <xref ref-type="bibr" rid="bib1.bibx27" id="paren.35"/> providing an estimate of the
alongshore profile of this mode.  They found a strong harmonic response
over the majority of the eastern bay shoreline with a damped response
in an area north of the submarine canyon.  Based on this, we estimate
that approximately 70 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of the shoreline responds to this
mode.  In the spirit of our gross estimate, we assume the alongshore
spatial dimension of the mode to be <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>≈</mml:mo><mml:mn>0.7</mml:mn><mml:mo>×</mml:mo><mml:mn>40</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">km</mml:mi><mml:mo>=</mml:mo><mml:mn>28</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>.  Combining this with the
cross-shore elevation area, we arrive at an estimate of the volume of
water displaced by this mode of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>≈</mml:mo><mml:mn>258</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Mm</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>.  The
energy to move this mass is equivalent to the work performed to change
the potential energy of the mass in the gravitational field, and we
estimate the energy of the mode as <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">ρ</mml:mi><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>h</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>g</mml:mi><mml:mo>≈</mml:mo><mml:mn>894.75</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">GJ</mml:mi></mml:math></inline-formula>, or
an average power of 406 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">MW</mml:mi></mml:math></inline-formula> over the 36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> modal
period.  Obviously, this leading-order value does not incorporate
dissipation and momentum, terms that we ignore in all subsequent
energy estimates.</p>
      <p>If the <inline-formula><mml:math display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> factor is
large (the resonance signal-to-noise ratio is high), then <inline-formula><mml:math display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> may be
estimated from the power spectrum: <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Q</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>f</mml:mi></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the mode resonant
frequency and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>f</mml:mi></mml:mrow></mml:math></inline-formula> the <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">dB</mml:mi></mml:math></inline-formula> (half power)
bandwidth of the mode.  We observe signal-to-noise ratios routinely
exceeding 5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">dB</mml:mi></mml:math></inline-formula> at the bay modes
(Figs. <xref ref-type="fig" rid="Ch1.F4"/> and
<xref ref-type="fig" rid="Ch1.F13"/>) and use PSD estimates based
on 120 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> records of 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> NTR (95 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> CI
2.6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">dB</mml:mi></mml:math></inline-formula>) advanced in 4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> increments to find a mean
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>f</mml:mi><mml:mo>=</mml:mo><mml:mn>5.86</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> and an estimate of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Q</mml:mi><mml:mo>=</mml:mo><mml:mn>7.74</mml:mn></mml:mrow></mml:math></inline-formula>
for the 36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> mode.  This implies that within the gross
level of estimation in which we are engaged, the driving energy for the
36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> mode is roughly <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>894.75</mml:mn><mml:mo>/</mml:mo><mml:mn>7.75</mml:mn><mml:mo>≈</mml:mo><mml:mn>115.5</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">GJ</mml:mi></mml:math></inline-formula>, or a power consumption of 52.4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">MW</mml:mi></mml:math></inline-formula>.  We will
compare this forcing to estimates of energy available from prospective
mode drivers in the following sections.</p>
<sec id="Ch1.S5.SS1.SSS1">
  <title>Microseisms</title>
      <p>Microseisms are pressure (acoustic) waves primarily generated by
nonlinear wave–wave interactions on the ocean surface.  They radiate
into the atmosphere where they are globally detected as microbaroms
<xref ref-type="bibr" rid="bib1.bibx33" id="paren.36"/>, into the water column as acoustic modes, and
couple into the seafloor where they travel as Rayleigh/Stoneley waves
presenting a global seismic signature <xref ref-type="bibr" rid="bib1.bibx34" id="paren.37"/>.  One can
estimate deep water microseismic energy by considering the acoustic
intensity of a plane wave incident on the seafloor
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msup><mml:mi>P</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>/</mml:mo><mml:mi>Z</mml:mi></mml:mrow></mml:math></inline-formula> where <inline-formula><mml:math display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> is the pressure
and <inline-formula><mml:math display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> the acoustic impedance.  In the linear regime, the
characteristic acoustic impedance of a medium is
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">ρ</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi>c</mml:mi></mml:mrow></mml:math></inline-formula> where <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ρ</mml:mi></mml:math></inline-formula> is the density and
<inline-formula><mml:math display="inline"><mml:mi>c</mml:mi></mml:math></inline-formula> the sound speed, which in the case of seawater is
approximately <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>≈</mml:mo><mml:mn>1.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">N</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">s</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>.
Spectral amplitudes of the microseism peak at deep water seafloor
sites were found by <xref ref-type="bibr" rid="bib1.bibx34" id="text.38"/> to be approximately
5000 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Pa</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">Hz</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, giving an intensity of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">W</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>.  Assuming a source generation
region of radius 100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>, the total power is 157 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">MW</mml:mi></mml:math></inline-formula>.</p>
      <p>This energy is efficiently converted into seismic Rayleigh waves or
ocean acoustic modes <xref ref-type="bibr" rid="bib1.bibx13" id="paren.39"/>, and these waves can
propagate with small attenuation coefficients over large distances,
suggesting that microseismic energy is of sufficient magnitude to
couple to bay resonances.  However, <xref ref-type="bibr" rid="bib1.bibx6" id="text.40"/> demonstrate
that coastal zone microseismic energy is dominated by local wave
reflections from coasts, not deep water arrivals, as propagation from
deep to shallow water is inhibited by the changing seismic waveguide
as refraction of the Rayleigh modes significantly reduces energy
reaching the coastal zone <xref ref-type="bibr" rid="bib1.bibx13" id="paren.41"/>.
<xref ref-type="bibr" rid="bib1.bibx6" id="text.42"/> found coastal zone pressures of approximately
<inline-formula><mml:math display="inline"><mml:mn>70</mml:mn></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Pa</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">Hz</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, which under the same assumptions as
the deep water case gives a total power of 2.2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">MW</mml:mi></mml:math></inline-formula>,
insufficient to drive the fundamental bay mode.  Not only is the
estimated energy insufficient, microseismic energy is distributed
around periods of 5 to 7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>, more than 2 orders of magnitude
shorter than the dominant bay mode, and we conclude that microseisms
are not a likely driving mechanism for the continuous bay
oscillations.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S5.SS1.SSS2">
  <title>Internal waves</title>
      <p><xref ref-type="bibr" rid="bib1.bibx18" id="text.43"/> observed that internal waves in Monterey Canyon are
nearly an order of magnitude more energetic than in the open ocean and
are tidally locked to <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.  Mean horizontal energy fluxes
are steered by canyon bathymetry and are predominantly up canyon, with
depth integrated fluxes of 5 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">kW</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> at the
mouth diminishing to <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">kW</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> near the head
(Moss Landing), although the internal wave field is highly anisotropic,
with evidence of both sources and sinks along the canyon.
Particularly energetic fluxes have been characterized as bores with
peak currents of  55 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">cm</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> averages
exceeding 30 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">cm</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx16" id="paren.44"/>.  <xref ref-type="bibr" rid="bib1.bibx7" id="text.45"/>
quantified turbulent kinetic energy dissipation, finding that the
turbulence is primarily in a stratified turbulent layer (STL) along
the canyon floor and is thickest on the canyon axis.  Time averaged
values of STL thickness and dissipation were estimated to be
135 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="italic">ε</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mn>1.36</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">kg</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>.</p>
      <p>Both <xref ref-type="bibr" rid="bib1.bibx18" id="text.46"/> and <xref ref-type="bibr" rid="bib1.bibx7" id="text.47"/> compared mean internal
wave energy flux with dissipation rates, tentatively concluding that
most of the along-canyon internal energy is dissipated as turbulence,
although <xref ref-type="bibr" rid="bib1.bibx7" id="text.48"/> noted that “large error estimates suggest
this agreement is fortuitous”.  A gross estimate of the internal tide
energy can be made from a mean value of energy flux:
2 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">kW</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx18" id="paren.49"/>, which for a 20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>
length of canyon gives <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">I</mml:mi></mml:msub><mml:mo>≈</mml:mo><mml:mn>40</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">MW</mml:mi></mml:math></inline-formula>
(20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> corresponds to the length of the canyon from the head over
which there is a primarily a single channel, is approximately equal to
the length of the primary transverse mode, and is the length used by
<xref ref-type="bibr" rid="bib1.bibx7" id="text.50"/> in their global estimates of canyon dissipation).
An estimate of the dissipation over this 20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> section with
a mean STL height of 135 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> and width of 4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mtext>STL</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mn>10.8</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Gm</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>) gives
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">ρ</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>V</mml:mi><mml:mtext>STL</mml:mtext></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mover accent="true"><mml:mi mathvariant="italic">ε</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>≈</mml:mo><mml:mn>15.1</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">MW</mml:mi></mml:math></inline-formula>.</p>
      <p>Even if these gross estimates of internal wave energy and dissipation,
which ignore the well-documented fine-scale sink/source and spatial
variability, are only accurate to a factor of 2, the residual energy
rate <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">I</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>40</mml:mn><mml:mo>-</mml:mo><mml:mn>15</mml:mn><mml:mo>=</mml:mo><mml:mn>25</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">MW</mml:mi></mml:math></inline-formula> is insufficient to sustain our estimate of the fundamental
mode (52.4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">MW</mml:mi></mml:math></inline-formula>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><caption><p><bold>(a)</bold> Wavelet level W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> of the nontide residual over
a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> period on 21 September 2013 when offshore wave height was
2.4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>. <bold>(b)</bold> Time series reconstruction from ten spectral
amplitudes of Fig. <xref ref-type="fig" rid="Ch1.F6"/> at periods of 58, 83, 94, 97,
100, 104, 107, 112, 116 and 209 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>.
</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f11.png"/>

          </fig>

</sec>
<sec id="Ch1.S5.SS1.SSS3">
  <title>Mesoscale eddy</title>
      <p>A potential energy source that, to the authors knowledge, has not been
considered as a mode driver, is the persistent mesoscale anticyclonic
gyre offshore Monterey Bay (Fig. <xref ref-type="fig" rid="Ch1.F2"/>).
The gyre is nominally 50–70 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> in
diameter and models suggest that it extends from the surface to at
least 600 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> in depth with instantaneous velocities of
70 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">cm</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> near the surface and 30 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">cm</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> at
depth <xref ref-type="bibr" rid="bib1.bibx30 bib1.bibx32" id="paren.51"/>.  The gyre supports a persistent
elevated dome of sea surface height (SSH) rising approximately
10–12 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula> above the coastal levels along the eastern shore of
the bay <xref ref-type="bibr" rid="bib1.bibx32" id="paren.52"/>.</p>
      <p>The potential energy of this dome with respect to the coast can be
estimated by assuming the dome has a cosine-bell profile from the
center with <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>≈</mml:mo><mml:mn>30</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>.  Taking the height of
the dome to be <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>h</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>10</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula>, the dome volume is
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">π</mml:mi><mml:msubsup><mml:mo>∫</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msubsup><mml:mo>[</mml:mo><mml:msub><mml:mi>h</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>h</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>x</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>k</mml:mi><mml:mi>x</mml:mi><mml:mo>)</mml:mo><mml:mo>]</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">d</mml:mi><mml:mi>x</mml:mi><mml:mo>=</mml:mo><mml:mn>168</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Mm</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> where
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">π</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:math></inline-formula>.  The potential energy of this mass is
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">ρ</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi>g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mfrac><mml:mrow><mml:msub><mml:mi>h</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msub></mml:mrow><mml:msqrt><mml:mn mathvariant="normal">2</mml:mn></mml:msqrt></mml:mfrac><mml:mo>=</mml:mo><mml:mn>120.7</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">GJ</mml:mi></mml:math></inline-formula>, which is comparable with the 115.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">GJ</mml:mi></mml:math></inline-formula>
estimated to sustain the 36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> fundamental mode.  However,
even though the geostrophic balance of the gyre will fluctuate due to
wind stress and dynamics of gyre interaction with the California
Current, it is unlikely that the geostrophic balance will fluctuate by
its full amplitude on timescales of 30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>, allowing this mass
of water to relax and propagate as a wave.</p>
      <p>The kinetic energy of the equatorward portion of the gyre can be
estimated from the cross-sectional flow of the gyre, which from the
model of <xref ref-type="bibr" rid="bib1.bibx30" id="text.53"/> during a weak flow regime (April) can be
represented as a velocity of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>u</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">cm</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> from
a depth of at least 200 to 600 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> over a width of
30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>.  A 30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> long section of this flow
(corresponding to the length of the equatorward portion of the gyre
just offshore the bay) would have a kinetic energy of
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi mathvariant="normal">K</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfrac><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">ρ</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">K</mml:mi></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi>u</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn>465.8</mml:mn></mml:mrow></mml:math></inline-formula>
<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">GJ</mml:mi></mml:math></inline-formula>, so there appears to be sufficient energy in the jet
offshore the bay to sustain the fundamental mode, but it is not clear
how a portion of this energy would couple into the mode.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><caption><p>Discrete wavelet transform decomposition of nontide residual water
level during a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> period with an offshore significant wave height of
2.0 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>. Dashed vertical lines mark periods of synchronization between
the W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>≈</mml:mo><mml:mn>118</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>) and W<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>≈</mml:mo><mml:mn>111</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>)
levels. </p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f12.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13"><caption><p><bold>(a)</bold> Spectrogram of 6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> water levels at the
Monterey tide gauge from August 1996 through June 2014. <bold>(b)</bold> Power
spectral density estimate of 6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> water levels at the Monterey tide
gauge from August 1996 through June 2014. Dashed vertical lines mark the
bay-wide resonance modes of 55.9, 36.7, 27.4, 21.8, 18.5 and
16.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>. </p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://os.copernicus.org/articles/11/439/2015/os-11-439-2015-f13.jpg"/>

          </fig>

      <p>One possibility is that the shear interface between the jet and deeper
water generates Kelvin–Helmholtz instabilities to drive the fundamental
mode.  With the assumption of two stratified water masses of density
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and mean velocities
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, the minimum horizontal
wave number of instabilities can be found from a dispersion relation of
the unsteady Bernoulli equation <xref ref-type="bibr" rid="bib1.bibx17" id="paren.54"/> as

                  <disp-formula id="Ch1.E3" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mtext>min</mml:mtext></mml:msub><mml:mo>&lt;</mml:mo><mml:mfrac><mml:mrow><mml:mi>g</mml:mi><mml:mfenced close=")" open="("><mml:msubsup><mml:mi mathvariant="italic">ρ</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi mathvariant="italic">ρ</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mfenced></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msup><mml:mfenced open="(" close=")"><mml:msub><mml:mi>U</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>U</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfrac><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p>To apply this, we assume that the upper water mass is the warmer,
fresher water of the California Current gyre (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>U</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) and the lower layer the colder, saltier deep water
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>U</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), where values of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn>1026.70</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">kg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn>1026.97</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">kg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> are mean values from the surface to a depth of
200 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> at offshore and canyon locations computed from
temperature and salinities reported in Fig. 13 of
<xref ref-type="bibr" rid="bib1.bibx26" id="text.55"/> using the method of <xref ref-type="bibr" rid="bib1.bibx12" id="text.56"/>.  The
resultant maximum wavelengths over the range of velocity differences
suggested by <xref ref-type="bibr" rid="bib1.bibx30" id="text.57"/> (30–70 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">cm</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>)
indicate that instabilities with length scales of several hundred
meters are possible.  However, these length scales are much shorter
than the characteristic scale of the 36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> fundamental bay
mode (26.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>), and it seems unlikely that even coherent
trains of such instabilities could effectively drive the fundamental
mode.</p>
      <p>Finally, we examined whether there was a relation between the seasonal
upwelling and mode response.  Upwelling in the bay typically peaks in
spring/summer (April/May), introducing a tongue of upwelled water
between the gyre and the outside edge of the bay.  It was assumed that,
if the bay modes are driven by the gyre, then upwelling that might
partially decouple the bay from the gyre could have an impact on the
bay mode amplitudes.  We compared PSD estimates of the 6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> data
averaged over 17 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">years</mml:mi></mml:math></inline-formula> for April and May with PSD estimates
from September and October, but found no statistically significant
differences.  To the extent that upwelling was expressed in the April
and May data, we find no evidence to support the idea that it changes
the oscillating modes.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <title>Conclusions</title>
      <p>Monterey Bay is an intensely studied oceanic body, with the Naval
Postgraduate School, Moss Landing Marine Laboratories, Hopkins Marine
Station and Monterey Bay Aquarium Research Institute providing decades
of physical oceanographic research.  Water level oscillations in the
bay have been studied since at least the late 1940s, yet it seems
that <xref ref-type="bibr" rid="bib1.bibx4" id="text.58"/> were the first to notice that bay-wide
oscillations are continuously present.  Based on a 17.8 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">year</mml:mi></mml:math></inline-formula>
record of water levels at the NOAA tide station, we substantiate their
observation and validate the accuracy of oscillation periods of the
six primary bay modes determined by <xref ref-type="bibr" rid="bib1.bibx5" id="text.59"/>.  Amplitudes
of the bay modes indicate that the fundamental transverse mode
(36.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>) is the mode that is most directly driven by the
unknown source.  Kinematics of this oscillation coupled with the
resonance amplitude lead us to estimate that a power source of roughly
52.4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">MW</mml:mi></mml:math></inline-formula> drives this mode.  Comparison of this energy rate to
prospective forcings from microseisms, internal waves and the
associated turbulence indicate that neither of these mechanisms has
sufficient power to sustain the mode.  We also find that surface waves
are not coherently related to the bay modes.</p>
      <p>A potential mode driver is the anticyclonic mesoscale gyre situated
just offshore the bay.  The potential and kinetic energy it contains
are sufficient to sustain the fundamental mode; however, we find that
turbulent instabilities such as Kelvin–Helmholtz waves generated in
the shear interface of the gyre do not have spatial scales consistent
with the fundamental mode.  It is intriguing to note that the nodal
line of the fundamental transverse mode would be located roughly
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>=</mml:mo><mml:mn>26.7</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> from the eastern shore, corresponding
roughly to the eastern edge of the gyre.  It would seem a peculiar
circumstance if this spatial arrangement along with the potential and
kinetic energy scales of the gyre were merely coincidental to the
continuous harmonic driver of bay modes, but presently we cannot
conceptualize a supportable mechanism for such a coupling.  While the
present study is purely observational, high-resolution non-hydrostatic
coupled ocean–atmosphere models could clarify the roles of potential
mode drivers, and should be pursued.</p>
      <p>Regarding oscillations in Monterey Harbor, we present the first high-resolution analysis resolving spectral components to periods as short
as 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>.  The spectral nature of these modes indicates that they
represent a continuum of harmonic oscillators closely spaced in
wave number.  For example, the 112 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula> dominant mode can be
attributed to standing waves between the tide gauge and multiple
boundaries including the rocky coast to the east, the breakwater to
the north and mooring docks to the northeast, while the 41 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula>
mode is associated with the breakwater to the south.  Concerning wave
forcing, it is demonstrated that the primary harbor mode amplitude
grows as the square root of offshore significant wave height, and that
there is a mode-specific dependence on wave-arrival direction.  It is
also observed that tidal phase serves to frequency modulate the harbor
modes, with evidence of enhanced mode energy during high tide.</p>
      <p>A temporal analysis monitoring the evolution of harbor modes in
response to wave forcing supports the idea that amplitude modulation
of specific harbor modes arises from modal interference, and it is
observed that when such modulations synchronize, they can have
a significant impact on water level amplitude.  Identification of
specific modes with associated physical sources raises the possibility
of engineering solutions to mitigate specific oscillations.</p><?xmltex \hack{\clearpage}?>
</sec>

      
      </body>
    <back><app-group><app id="App1.Ch1.S1">
  <title/>
      <p>The maximal overlap discrete wavelet transform (MODWT,
<xref ref-type="bibr" rid="bib1.bibx23" id="altparen.60"/>) is defined by

              <disp-formula id="App1.Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mi>j</mml:mi><mml:mi>J</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="bold-italic">D</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">S</mml:mi><mml:mi>J</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

        where <inline-formula><mml:math display="inline"><mml:mi mathvariant="bold-italic">X</mml:mi></mml:math></inline-formula> is a time series of length <inline-formula><mml:math display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula>
and <inline-formula><mml:math display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> represents a distinct wavelet level. The
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">D</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are referred to as wavelet details, and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">S</mml:mi><mml:mi>J</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> the smooth, each a vector of length <inline-formula><mml:math display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula>. The
details capture transient and oscillatory behavior at different
timescales; the smooth are the residual energy not captured by the
details and, in the optimal decomposition, correspond to a moving
average of the signal.  Each wavelet level is computed with a matrix
transform <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">D</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msubsup><mml:mi mathvariant="bold">W</mml:mi><mml:mi>j</mml:mi><mml:mi>T</mml:mi></mml:msubsup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="bold">Φ</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">S</mml:mi><mml:mi>J</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msubsup><mml:mi mathvariant="bold">V</mml:mi><mml:mi>j</mml:mi><mml:mi>T</mml:mi></mml:msubsup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="bold">Ψ</mml:mi><mml:mi>J</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> where <inline-formula><mml:math display="inline"><mml:mi mathvariant="bold">W</mml:mi></mml:math></inline-formula>
and <inline-formula><mml:math display="inline"><mml:mi mathvariant="bold">V</mml:mi></mml:math></inline-formula> are <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>×</mml:mo><mml:mi>N</mml:mi></mml:mrow></mml:math></inline-formula> matrices of MODWT
coefficients, and <inline-formula><mml:math display="inline"><mml:mi mathvariant="bold">Φ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi mathvariant="bold">Ψ</mml:mi></mml:math></inline-formula>
are referred to as the wavelet coefficient and scaling coefficient
vectors, respectively.  The wavelet and scaling coefficients are the
result of cascaded high-pass (<inline-formula><mml:math display="inline"><mml:mi>h</mml:mi></mml:math></inline-formula>) or low-pass (<inline-formula><mml:math display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula>)
wavelet and scaling filters recursively applied to the input
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">Φ</mml:mi><mml:mrow><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>l</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:msub><mml:mi>h</mml:mi><mml:mrow><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi></mml:mrow></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mtext>mod</mml:mtext><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>N</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, or
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">Ψ</mml:mi><mml:mrow><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>l</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:msub><mml:mi>g</mml:mi><mml:mrow><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi></mml:mrow></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mtext>mod</mml:mtext><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>N</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, where the
filter width at each level <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msup><mml:mn mathvariant="normal">2</mml:mn><mml:mi>j</mml:mi></mml:msup><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo><mml:mo>(</mml:mo><mml:mi>L</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> is
determined by the length of the mother wavelet <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">L</mml:mi></mml:math></inline-formula>. In terms
of the MODWT matrix and wavelet scaling coefficients, the
input can then be represented as

              <disp-formula id="App1.Ch1.E2" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mi>j</mml:mi><mml:mi>J</mml:mi></mml:munderover><mml:msubsup><mml:mi mathvariant="bold">W</mml:mi><mml:mi>j</mml:mi><mml:mi>T</mml:mi></mml:msubsup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="bold">Φ</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="bold">V</mml:mi><mml:mi>J</mml:mi><mml:mi>T</mml:mi></mml:msubsup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="bold">Ψ</mml:mi><mml:mi>J</mml:mi></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p>The MODWT provides a convenient encapsulation of the signal energy in
terms of the wavelet and scaling coefficient vectors:

              <disp-formula id="App1.Ch1.E3" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mo>‖</mml:mo><mml:mi mathvariant="bold-italic">X</mml:mi><mml:msup><mml:mo>‖</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mi>j</mml:mi><mml:mi>J</mml:mi></mml:munderover><mml:mo>‖</mml:mo><mml:msub><mml:mi mathvariant="bold">Φ</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:msup><mml:mo>‖</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mo>‖</mml:mo><mml:msub><mml:mi mathvariant="bold">Ψ</mml:mi><mml:mi>J</mml:mi></mml:msub><mml:msup><mml:mo>‖</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

        which is related to the sample variance of <inline-formula><mml:math display="inline"><mml:mi mathvariant="bold-italic">X</mml:mi></mml:math></inline-formula>.  It
is useful to plot the wavelet coefficients of each level scaled by its
respective magnitude squared so that the relative amplitude scales
represent the partial variance contributed by each level.</p><?xmltex \hack{\clearpage}?>
</app>
  </app-group><ack><title>Acknowledgements</title><p>The authors gratefully acknowledge insightful discussions and reviews of the
manuscript by L. Breaker of Moss Landing Marine Laboratory, University of
California, and Y.-H. Tseng, National Center for Atmospheric Research (NCAR)
Earth Systems Laboratory.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by:
E. J. M. Delhez</p></ack><ref-list>
    <title>References</title>

      <ref id="bib1.bibx1"><label>AMS(1903)</label><mixed-citation>AMS: Seiches in Lake Garda, Mon. Weather Rev., 31, 532–533,
doi:<ext-link xlink:href="http://dx.doi.org/10.1175/1520-0493(1903)31[532b:SILG]2.0.CO;2">10.1175/1520-0493(1903)31[532b:SILG]2.0.CO;2</ext-link>, 1903.</mixed-citation></ref>
      <ref id="bib1.bibx2"><label>AMS(1906)</label><mixed-citation>AMS: The seiche and its mechanical explanation, Mon. Weather Rev., 34,
226,
doi:<ext-link xlink:href="http://dx.doi.org/10.1175/1520-0493(1906)34&lt;226b:TSAIME&gt;2.0.CO;2">10.1175/1520-0493(1906)34&lt;226b:TSAIME&gt;2.0.CO;2</ext-link>, 1906.</mixed-citation></ref>
      <ref id="bib1.bibx3"><label>Bloomfield(1976)</label><mixed-citation>
Bloomfield, P.: Fourier Analysis of Time Series: An Introduction, Wiley, New York,
1st Edn., 261 pp., 1976.</mixed-citation></ref>
      <ref id="bib1.bibx4"><label>Breaker et al.(2008)Breaker, Broenkow, Watson, and Jo</label><mixed-citation>
Breaker, L. C., Broenkow, W. W., Watson, W. E., and Jo, Y.: Tidal and non-tidal
oscillations in Elhorn Slough, California, Estuar. Coast., 31,
239–257, 2008.</mixed-citation></ref>
      <ref id="bib1.bibx5"><label>Breaker et al.(2010)Breaker, Tseng, and Wang</label><mixed-citation>Breaker, L. C., Tseng, Y., and Wang, X.: On the natural oscillations of
Monterey Bay: observations, modeling, and origins, Prog. Oceanogr., 86, 380–395,
doi:<ext-link xlink:href="http://dx.doi.org/10.1016/j.pocean.2010.06.001">10.1016/j.pocean.2010.06.001</ext-link>, 2010.</mixed-citation></ref>
      <ref id="bib1.bibx6"><label>Bromirski and Duennebier(2002)</label><mixed-citation>Bromirski, P. D. and Duennebier, F. K.: The near-coastal microseism spectrum:
spatial and temporal wave climate relationships, J. Geophys. Res.-Sol. Ea., 107, ESE 5-1–ESE 5-20,
doi:<ext-link xlink:href="http://dx.doi.org/10.1029/2001JB000265">10.1029/2001JB000265</ext-link>, 2002.</mixed-citation></ref>
      <ref id="bib1.bibx7"><label>Carter and Gregg(2002)</label><mixed-citation>Carter, G. S. and Gregg, M. C.: Intense, variable mixing near the head of
Monterey Submarine Canyon, J. Phys. Oceanogr., 32, 3145–3165,
doi:<ext-link xlink:href="http://dx.doi.org/10.1175/1520-0485(2002)032&lt;3145:IVMNTH&gt;2.0.CO;2">10.1175/1520-0485(2002)032&lt;3145:IVMNTH&gt;2.0.CO;2</ext-link>, 2002.</mixed-citation></ref>
      <ref id="bib1.bibx8"><label>CDIP(2014)</label><mixed-citation>CDIP: Station 156 Monterey Canyon Outer, available at:
<uri>http://cdip.ucsd.edu/?nav=recent&amp;stn=156&amp;sub=observed&amp;xitem=info&amp;stream=p1</uri>,
last access: 14 November 2014.</mixed-citation></ref>
      <ref id="bib1.bibx9"><label>Chrystal(1906)</label><mixed-citation>Chrystal, G.: On the hydrodynamical theory of seiches, T. Roy. Soc. Edin.-Earth, 41, 599–649,
doi:<ext-link xlink:href="http://dx.doi.org/10.1017/S0080456800035523">10.1017/S0080456800035523</ext-link>,
1906.</mixed-citation></ref>
      <ref id="bib1.bibx10"><label>Darwin(1899)</label><mixed-citation>
Darwin, G. H.: The Tides and Kindred Phenomena in the Solar System, Houghton,
Boston, 342 pp., 1899.</mixed-citation></ref>
      <ref id="bib1.bibx11"><label>Forston et al.(1949)Forston, Brown, Hudson, Wilson, and
Bell</label><mixed-citation>
Forston, E. P., Brown, F. R., Hudson, R. Y., Wilson, H. B., and Bell, H. A.:
Wave and surge action, Monterey Harbor, Monterey California, Tech.
Rep. 2-301, United States Army Corps of Engineers, Waterways Experiment
Station, Vicksburg, MS, 45 Plates, 1949.</mixed-citation></ref>
      <ref id="bib1.bibx12"><label>Gill(1982)</label><mixed-citation>
Gill, A. E.: Atmosphere-Ocean Dynamics, Academic Press, New York, 662 pp., 1982.</mixed-citation></ref>
      <ref id="bib1.bibx13"><label>Hasselmann(1963)</label><mixed-citation>Hasselmann, K.: A statistical analysis of the generation of microseisms,
Rev. Geophys., 1, 177–210,
doi:<ext-link xlink:href="http://dx.doi.org/10.1029/RG001i002p00177">10.1029/RG001i002p00177</ext-link>, 1963.</mixed-citation></ref>
      <ref id="bib1.bibx14"><label>IOOS(2009)</label><mixed-citation>IOOS: A National Operational Wave Observation Plan. Integrated Ocean Observing
System (IOOS) plan for a surface-wave monitoring network for the United
States, Tech. rep., Integrated Ocean Observing System, available at:
<uri>http://www.ioos.noaa.gov/library/wave_plan_final_03122009.pdf</uri> (last access: 14 November 2014), 2009.
</mixed-citation></ref><?xmltex \hack{\newpage}?>
      <ref id="bib1.bibx15"><label>Kedar et al.(2008)Kedar, Longuet-Higgins, Webb, Graham, Clayton, and
Jones</label><mixed-citation>Kedar, S., Longuet-Higgins, M., Webb, F., Graham, N., Clayton, R., and Jones, C.: The origin of deep ocean microseisms in the North Atlantic Ocean, P. R. Soc. A, 464, 777–793,
doi:<ext-link xlink:href="http://dx.doi.org/10.1098/rspa.2007.0277">10.1098/rspa.2007.0277</ext-link>,
2008.</mixed-citation></ref>
      <ref id="bib1.bibx16"><label>Key(1999)</label><mixed-citation>Key, S. A.: Internal tidal bores in the Monterey Canyon, M. S. thesis,
Naval Postgraduate School, available at:  <uri>http://www.dtic.mil/dtic/tr/fulltext/u2/a370949.pdf</uri> (last access; 14 November 2014),
1999.</mixed-citation></ref>
      <ref id="bib1.bibx17"><label>Kundu(1990)</label><mixed-citation>
Kundu, P. K.: Fluid Mechanics, Academic Press, San Diego, 1st Edn., 638 pp., 1990.</mixed-citation></ref>
      <ref id="bib1.bibx18"><label>Kunze et al.(2002)Kunze, Rosenfeld, Carter, and Gregg</label><mixed-citation>Kunze, E., Rosenfeld, L. K., Carter, G. S., and Gregg, M. C.: Internal waves in
Monterey Submarine Canyon, J. Phys. Oceanogr., 32, 1890–1913,
doi:<ext-link xlink:href="http://dx.doi.org/10.1175/1520-0485(2002)032&lt;1890:IWIMSC&gt;2.0.CO;2">10.1175/1520-0485(2002)032&lt;1890:IWIMSC&gt;2.0.CO;2</ext-link>, 2002.</mixed-citation></ref>
      <ref id="bib1.bibx19"><label>NOAA(2014a)</label><mixed-citation>NOAA: Monterey, CA, National Water Level Observation Network –
Station ID: 9413450, available at:
<uri>http://tidesandcurrents.noaa.gov/stationhome.html?id=9413450</uri>, last
access: 14 November  2014a.</mixed-citation></ref>
      <ref id="bib1.bibx20"><label>NOAA(2014b)</label><mixed-citation>NOAA: Harmonic Constituents for 9413450, Monterey CA,
available at:  <uri>http://tidesandcurrents.noaa.gov/harcon.html?id=9413450</uri>,
last access: 14 November  2014b.</mixed-citation></ref>
      <ref id="bib1.bibx21"><label>Park et al.(2014)Park, Heitsenrether, and Sweet</label><mixed-citation>
Park, J., Heitsenrether, R., and Sweet, W.: Microwave and acoustic water level
and significant wave height estimates at NOAA tide stations, J. Atmos. Ocean. Tech., 31, 2294–2308, 2014.</mixed-citation></ref>
      <ref id="bib1.bibx22"><label>Parke and Gill(1995)</label><mixed-citation>
Parke, M. E. and Gill, S. K.: On the sea state dependence of sea level
measurements at platform Harvest, Mar. Geod., 18, 105–111, 1995.</mixed-citation></ref>
      <ref id="bib1.bibx23"><label>Percival and Walden(2006)</label><mixed-citation>
Percival, D. B. and Walden, A. T.: Wavelet Methods for Time Series Analysis,
Cambridge University Press, New York, 594 pp., 2006.</mixed-citation></ref>
      <ref id="bib1.bibx24"><label>Petruncio et al.(1998)Petruncio, Rosenfeld, and
Paduan</label><mixed-citation>Petruncio, E., Rosenfeld, L., and Paduan, P.: Observations of the internal tide
in Monterey Canyon, J. Phys. Oceanogr., 28, 1873–1903,
doi:<ext-link xlink:href="http://dx.doi.org/10.1175/1520-0485(1998)028&lt;1873:OOTITI&gt;2.0.CO;2">10.1175/1520-0485(1998)028&lt;1873:OOTITI&gt;2.0.CO;2</ext-link>, 1998.</mixed-citation></ref>
      <ref id="bib1.bibx25"><label>Raines(1967)</label><mixed-citation>Raines, W. A.: Sub-tidal oscillations in Monterey Harbor, M. S. thesis,
Naval Postgraduate School, available at:   <uri>https://calhoun.nps.edu/bitstream/handle/10945/13214/subtidaloscillat00bain.pdf?sequence=1</uri>  (last access: 4 June 2015),
1967.</mixed-citation></ref>
      <ref id="bib1.bibx26"><label>Rosenfeld et al.(1994)Rosenfeld, Schwing, Garfield, and
Tracy</label><mixed-citation>Rosenfeld, L. K., Schwing, F. B., Garfield, N., and Tracy, D. E.: Bifurcated
flow from an upwelling center: a cold water source for Monterey Bay,
Cont. Shelf. Res., 14, 931–964,
doi:<ext-link xlink:href="http://dx.doi.org/10.1016/0278-4343(94)90058-2">10.1016/0278-4343(94)90058-2</ext-link>, 1994.</mixed-citation></ref>
      <ref id="bib1.bibx27"><label>Shchepetkin and McWilliams(2005)</label><mixed-citation>Shchepetkin, A. F. and McWilliams, J. C.: The regional oceanic modeling system
(ROMS): a split-explicit, free-surface, topography-following-coordinate
oceanic model, Ocean Model., 9, 347–404,
doi:<ext-link xlink:href="http://dx.doi.org/10.1016/j.ocemod.2004.08.002">10.1016/j.ocemod.2004.08.002</ext-link>, 2005.</mixed-citation></ref>
      <ref id="bib1.bibx28"><label>Ryan et al.(2014)Davis, Tufillaro, Kudela and Gao</label><mixed-citation>Ryan, J. P., Davis, C. O., Tufillaro, N. B., Kudela, R. M. and Gao, B. C.:
Application of the Hyperspectral Imager for the Coastal Ocean to Phytoplankton  Ecology Studies in Monterey Bay, CA, USA,
Remote Sens., 6, 1007–1025,
doi:<ext-link xlink:href="http://dx.doi.org/10.3390/rs6021007">10.3390/rs6021007</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bibx29"><label>Strub et al.(1991)Strub, Kosro, and Huyer</label><mixed-citation>Strub, P. T., Kosro, P. M., and Huyer, A.: The nature of the cold filaments in
the California Current system, J. Geophys. Res.-Oceans,
96, 14743–14768,
doi:<ext-link xlink:href="http://dx.doi.org/10.1029/91JC01024">10.1029/91JC01024</ext-link>, 1991.</mixed-citation></ref>
      <ref id="bib1.bibx30"><label>Tseng and Breaker(2007)</label><mixed-citation>Tseng, Y.-H. and Breaker, L. C.: Nonhydrostatic simulations of the regional
circulation in the Monterey Bay area, J. Geophys. Res.-Oceans, 112, C12017,
doi:<ext-link xlink:href="http://dx.doi.org/10.1029/2007JC004093">10.1029/2007JC004093</ext-link>, 2007.</mixed-citation></ref>
      <ref id="bib1.bibx31"><label>Tseng et al.(2005)Tseng, Dietrich, and Ferziger</label><mixed-citation>Tseng, Y.-H., Dietrich, D. E., and Ferziger, J. H.: Regional circulation of the
Monterey Bay region: hydrostatic versus nonhydrostatic modeling,
J. Geophys. Res.-Oceans, 110, C09015,
doi:<ext-link xlink:href="http://dx.doi.org/10.1029/2003JC002153">10.1029/2003JC002153</ext-link>, 2005.</mixed-citation></ref>
      <ref id="bib1.bibx32"><label>Tseng et al.(2012)Tseng, Chien, Jin, and Miller</label><mixed-citation>Tseng, Y.-H., Chien, S.-H., Jin, J., and Miller, N. L.: Modeling air-land-sea interactions using the integrated regional model system in
Monterey Bay, California, Mon. Weather Rev., 140, 1285–1306,
doi:<ext-link xlink:href="http://dx.doi.org/10.1175/MWR-D-10-05071.1">10.1175/MWR-D-10-05071.1</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bibx33"><label>Waxler and Gilbert(2006)</label><mixed-citation>Waxler, R. and Gilbert, K. E.: The radiation of atmospheric microbaroms by
ocean waves,  J. Acoust. Soc.  Am., 119,
2651–2664,
doi:<ext-link xlink:href="http://dx.doi.org/10.1121/1.2191607">10.1121/1.2191607</ext-link>, 2006.
</mixed-citation></ref><?xmltex \hack{\newpage}?>
      <ref id="bib1.bibx34"><label>Webb and Cox(1986)</label><mixed-citation>Webb, S. C. and Cox, C. S.: Observations and modeling of seafloor microseisms,
J. Geophys. Res.-Sol. Ea., 91, 7343–7358,
doi:<ext-link xlink:href="http://dx.doi.org/10.1029/JB091iB07p07343">10.1029/JB091iB07p07343</ext-link>, 1986.</mixed-citation></ref>
      <ref id="bib1.bibx35"><label>Wilson et al.(1965)Wilson, Hendrickson, and Kilmer</label><mixed-citation>
Wilson, B. W., Hendrickson, J. A., and Kilmer, R. E.: Feasibility study for a
surge-action model of Monterey Harbor, California, Tech. Rep. 2–136,
United States Army Corps of Engineers, Waterways Experiment Station,
Vicksburg, MS, 1965.</mixed-citation></ref>

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