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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 Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/os-15-1091-2019</article-id><title-group><article-title>On the resolutions of ocean altimetry maps</article-title><alt-title>On the resolutions of ocean altimetry maps</alt-title>
      </title-group><?xmltex \runningtitle{On the resolutions of ocean altimetry maps}?><?xmltex \runningauthor{M.~Ballarotta et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Ballarotta</surname><given-names>Maxime</given-names></name>
          <email>mballarotta@groupcls.com</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Ubelmann</surname><given-names>Clément</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Pujol</surname><given-names>Marie-Isabelle</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Taburet</surname><given-names>Guillaume</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Fournier</surname><given-names>Florent</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4487-6082</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Legeais</surname><given-names>Jean-François</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Faugère</surname><given-names>Yannice</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3764-1429</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Delepoulle</surname><given-names>Antoine</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Chelton</surname><given-names>Dudley</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Dibarboure</surname><given-names>Gérald</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3644-2495</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Picot</surname><given-names>Nicolas</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Collecte Localisation Satellites, 31520 Ramonville-Saint-Agne, France</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>College of Earth, Ocean and Atmospheric Sciences, Oregon State
University, Corvallis, OR, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Centre National d'Études Spatiales, 31400 Toulouse, France</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Maxime Ballarotta (mballarotta@groupcls.com)</corresp></author-notes><pub-date><day>20</day><month>August</month><year>2019</year></pub-date>
      
      <volume>15</volume>
      <issue>4</issue>
      <fpage>1091</fpage><lpage>1109</lpage>
      <history>
        <date date-type="received"><day>21</day><month>December</month><year>2018</year></date>
           <date date-type="rev-request"><day>7</day><month>January</month><year>2019</year></date>
           <date date-type="rev-recd"><day>12</day><month>July</month><year>2019</year></date>
           <date date-type="accepted"><day>16</day><month>July</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 </copyright-statement>
        <copyright-year>2019</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://os.copernicus.org/articles/.html">This article is available from https://os.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://os.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://os.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e185">The Data Unification and Altimeter Combination System (DUACS) produces sea level global and regional
maps that serve oceanographic applications, climate forecasting centers,
and geophysics and biology communities. These maps are generated using an
optimal interpolation method applied to altimeter observations. They are
provided on a global <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M3" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (longitude <inline-formula><mml:math id="M6" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> latitude) and daily grid resolution framework
(<inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M9" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M11" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude <inline-formula><mml:math id="M12" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> latitude grid for the regional products) through the Copernicus Marine Environment Monitoring Service (CMEMS). Yet, the dynamical content of these maps does not have full <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> spatial and 1 d temporal resolutions due to the
filtering properties of the optimal interpolation. In the present study, we
estimate the effective spatial and temporal resolutions of the newly
reprocessed delayed-time DUACS maps (a.k.a. DUACS-DT2018). Our approach is
based on the ratio between the spectral content of the mapping error and the
spectral content of independent true signals (along-track and tide gauge
observations), also known as the noise-to-signal ratio. We found that the
spatial resolution of the DUACS-DT2018 global maps based on sampling by
three altimeters simultaneously ranges from <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> km wavelength
at high latitude to <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">800</mml:mn></mml:mrow></mml:math></inline-formula> km wavelength in the equatorial band
and the mean temporal resolution is <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">34</mml:mn></mml:mrow></mml:math></inline-formula> d. The mean
effective spatial resolution at midlatitude is estimated to be <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> km. The mean effective spatial resolution is <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">130</mml:mn></mml:mrow></mml:math></inline-formula> km for
the regional Mediterranean Sea and for the regional Black Sea products. An
intercomparison with previous DUACS reprocessing systems (a.k.a., DUACS-DT2010
and DUACS-DT2014) highlights the progress of the system over the past 8 years, in particular a gain of resolution in highly turbulent regions. The same diagnostic applied to maps constructed with two altimeters and maps with three altimeters confirms a modest increase in resolving capabilities and accuracies in the DUACS maps with the number of missions.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e377">The Data Unification and Altimeter Combination System (DUACS) generates, as
part of the CNES/SALP project and the Copernicus Marine Environment and
Monitoring Service (CMEMS), delayed-time (DT) multi-mission altimeter sea
level anomaly (SLA) level 3 (along-track cross-calibrated) and level 4
(multiple sensors merged as maps or time series) products. A full
reprocessing of these products is carried out approximately every 3 years
and covers the period 1993–now. The reprocessing benefits from
improvements associated with optimized mapping parameters and new altimeter
corrections which are based on standards recommended for altimeter products
by the different agencies and expert groups (Ocean Surface Topography
Science Team – OSTST, the ESA Quality Working Group and the ESA Sea Level
Climate Change Initiative project members). The previous reprocessing was
released in 2014 (DUACS-DT2014; see Pujol et al., 2016) and the new release,
namely DUACS-DT2018, is available since April 2018 (Taburet et al., 2019).</p>
      <?pagebreak page1092?><p id="d1e380">The level 4 DUACS-DT global maps are constructed from optimal interpolation
(Bretherton et al., 1976; Le Traon et al., 1998; Ducet et al., 2000) of level 3 altimeter observations and are provided on a regular <inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M22" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude <inline-formula><mml:math id="M25" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> latitude and daily grid resolution framework (<inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M28" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> horizontal sampling for the regional Mediterranean and Black Sea products). However, the optimal interpolation used in DUACS does not allow the restitution of the full dynamical spectrum of the ocean, limiting the capability of retrieving small mesoscale in level 4 products (Chelton et al., 2011, 2014).</p>
      <p id="d1e485">The effective resolution corresponds to the spatiotemporal scales of
the features that can be properly resolved in the maps. The spatiotemporal
resolution of the previous level 4 global SLA products was estimated by
Chelton et al. (2011, 2014) and Chelton and Schlax (2003) based on estimates of the mapping errors in sea surface height (SSH) fields constructed from altimeter data or spectral ratio analysis between maps and along-track altimeter data. Their analysis suggested a midlatitude spatial resolution capability of the observations ranging from <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> to 6<inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>,
depending on the number of altimeters used in the merging and the sampling
pattern of the ground track (<inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> for tandem mission T/P-Jason 5 d offset between parallel tracks, 6<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> for T/P mono-mission merging). The temporal resolution capability of the observations for a tandem T/P-Jason mission was estimated to be <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> d.</p>
      <p id="d1e544">In the present study, we further investigate the effective resolution of the
DUACS-DT gridded products using a spectral approach. The objective of the
paper is threefold: (1) to deliver the spatial distribution of the effective
resolutions as key information to the users about the quality and the
limitations (in term of resolution) of the newly produced DUACS-DT2018
gridded products, (2) to access and compare the spatial and temporal
resolution capabilities of the DUACS-DT2018, DUACS-DT2014 and DUACS-DT2010
maps (i.e., to identify the impact of system upgrades), and (3) to verify the
impact of the varying satellite constellation on the effective resolutions
of the maps. The paper is organized as follows. The data and method are
introduced in Sect. 2. In Sect. 3, we present our results. Finally, a
discussion and a conclusion are provided in Sect. 4. A sensitivity study
on the choice of spectral criterion to estimate the resolution and a comparison
of various approaches to estimate the resolution is given in the appendices.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and method</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Input data</title>
      <p id="d1e562">In the present study, we consider two kinds of data.
<list list-type="bullet"><list-item>
      <p id="d1e567"><italic>Independent dataset.</italic> we used two independent (i.e., not used in the mapping) datasets to evaluate the effective resolutions of the maps:
(1) level 3 CMEMS SLA from independent 1 Hz along-track data and (2) the SLA estimated from tide gauges. The along-track SLAs are constructed using a procedure similar to level 3 CMEMS products and are used to estimate the effective spatial resolution. The SLAs at tide gauge locations originate from the Global Sea Level Observing System and Climate and Ocean Variability, Predictability and Change (GLOSS-CLIVAR) network and are used to estimate the effective temporal resolution. GLOSS-CLIVAR data are worldwide and available with daily sampling.</p></list-item><list-item>
      <p id="d1e573">The maps of SLA are constructed using optimal interpolation, based on the a priori statistical knowledge of the field (e.g., variance, correlation scales, noise). The mapping procedure is based on merging of calibrated multi-satellite altimeter (level 3) data and follows the same protocol as described by Pujol et al. (2016) for the DUACS-DT2014. Taburet et al. (2019) give the full description and validation of the DUACS-DT2018 global and regional products. The main differences between the DUACS-DT2014 and the DUACS-DT2018 processing consist of an improved along-track processing (e.g., improved orbit correction, wet troposphere correction, ocean tide correction and a new mean sea surface) and updated a priori knowledge of the SLA variance and optimized selection of the data in the optimal interpolation. The maps tested here are computed specifically for this study in several constellation scenarios, keeping at least one mission out to allow an independent assessment of the resolution. The DUACS-DT products, formerly known as AVISO products, are referenced in the CMEMS catalogue as “OCEAN GRIDDED L3/4 SEA SURFACE HEIGHTS AND DERIVED VARIABLES REPROCESSED” products.</p></list-item></list></p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Method</title>
      <p id="d1e584">Our method to estimate the effective spatial resolution is based on the
ratio between the spectral content of the mapping error and the spectral
content of independent signals (along-track observations previously
mentioned).
            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M37" display="block"><mml:mrow><mml:mi mathvariant="normal">NSR</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">diff</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the spatial wavelength, <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">diff</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the power spectral density of the difference (SLA<inline-formula><mml:math id="M40" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">obs</mml:mi></mml:msub></mml:math></inline-formula>–SLA<inline-formula><mml:math id="M41" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">map</mml:mi></mml:msub></mml:math></inline-formula>) and <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the spectral density of the
independent observation.</p>
      <p id="d1e704">The algorithm to compute the spatial effective resolution follows four main
steps:
<list list-type="bullet"><list-item>
      <p id="d1e709">A coastal editing is applied in a 100 km coastal band (only for the global products) to remove the increased errors in the coastal area.</p></list-item><list-item>
      <p id="d1e713">Gridded data are interpolated to the locations of the independent along-track data.</p></list-item><list-item>
      <p id="d1e717">Along-track and interpolated data are divided into overlapping 1500 km long segments every 300 km for the<?pagebreak page1093?> global products (500 km long segments for the Mediterranean Sea products and 300 km long segments for the Black sea products). Each segment is saved in a database and referenced by its median (longitude, latitude) coordinates.</p></list-item><list-item>
      <p id="d1e721">Finally, between latitudes 90–90<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S and longitudes 0–360<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, we consider 10<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M46" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude <inline-formula><mml:math id="M48" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> latitude boxes for the global products (5<inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M50" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5<inline-formula><mml:math id="M51" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude <inline-formula><mml:math id="M52" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> latitude boxes for the Mediterranean Sea product, and 3<inline-formula><mml:math id="M53" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M54" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude <inline-formula><mml:math id="M56" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> latitude boxes for the Black Sea product) every 1<inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> incremental step. All available segments referenced within the 10<inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M59" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> box are selected to compute the power spectral densities based on the Welch (1967) method. Prior to spectral computation, signals are detrended and we applied a Hanning window. The effective resolution is then given by the wavelength <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> where the NSR(<inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is 0.5.</p></list-item></list>
The method (applied to the altimetry product) is illustrated in Fig. 1
with the data selection and interpolation step for the spectral analysis. The
total number of averaged segments in each 1<inline-formula><mml:math id="M63" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M64" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
longitude <inline-formula><mml:math id="M66" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> latitude box is shown in Fig. A1a for the global product, Fig. A1b for the Mediterranean Sea product and the Black Sea product. Due to the coastal editing, the number of computed segments in the global product analysis is less than 1000 near the coast and <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1500</mml:mn></mml:mrow></mml:math></inline-formula> in the open ocean. In the Mediterranean Sea the number of segments is
<inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">400</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">250</mml:mn></mml:mrow></mml:math></inline-formula>, respectively, for the Black Sea. A limitation of the present spectral approach is the need to rely on coastal data for estimation of the resolution in the two regional products. It is worth noting that we probably underestimate the resolution capability of the maps since we are estimating the spatial effective resolution of degraded maps to keep an independent dataset aside.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e963">Schematic illustration of the methodology: <bold>(a)</bold> input data selection, <bold>(b)</bold> co-location of SLA and gridded SLA and <bold>(c)</bold> spectral analysis showing the ratio error spectrum to signal spectrum.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f01.jpg"/>

        </fig>

      <p id="d1e982">A comparison of SLA maps with an independent tide gauge dataset is carried out
to estimate the effective temporal resolution. The approach is like the
estimate of the effective spatial resolution and based on the computation of
the ratio between the spectral content of the mapping error and the spectral
content of the true tide gauge signal (Eq. 2):
            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M70" display="block"><mml:mrow><mml:mi mathvariant="normal">NSR</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">diff</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the temporal wavelength, <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">diff</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the power spectral density of the difference (SLA<inline-formula><mml:math id="M73" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">obs</mml:mi></mml:msub></mml:math></inline-formula>–SLA<inline-formula><mml:math id="M74" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">map</mml:mi></mml:msub></mml:math></inline-formula>) and <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the spectral density of the
independent observation.</p>
      <p id="d1e1102">We computed the effective temporal resolution from each tide gauge time
series of the GLOSS-CLIVAR network. The temporal domain covers the period
1 January 1993–31 December 2015. The computation for each time series follows three main steps:
<list list-type="bullet"><list-item>
      <p id="d1e1107">At each tide gauge location, we extract the gridded SLA time series that is most highly correlated with tide gauge time series (note that the maximum distance separation of the grid point that is most highly correlated with each tide gauge is 100 km on average and can be as large as 300 km)</p></list-item><list-item>
      <p id="d1e1111">Each highly correlated time series (based on correlation criterion <inline-formula><mml:math id="M76" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.8) is subsampled into 365 d segments to compute the spectral densities <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The length of each segment must be set when estimating power spectral density using Welch's method. By subsampling into 365 d segments, we limit the frequency range to only periods shorter than 365 d. Note that consideration of time series longer than 365 d reduced the number of realizations because of occasional gaps in some of the data records. This can have an impact on the local estimation of the effective temporal resolution, e.g., from 365 d to 2-year segments we lose some continuous time series that do not contain a <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">365</mml:mn></mml:mrow></mml:math></inline-formula> d segment. In these cases, the spectral analysis cannot be performed.</p></list-item><list-item>
      <p id="d1e1154">The effective temporal resolution at each tide gauge location is given by the period <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> where the ratio NSR(<inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is equal to 0.5 (deduced by linear interpolation between successive NSR values).</p></list-item></list>
Note that this estimation of the temporal resolution is subject to an
important caveat: the estimation is based mainly on coastal locations which
may be contaminated by altimetry errors. Additionally, it may not be
fully representative of the temporal resolution of the DUACS maps which
combine various oceanic regimes (e.g., coastal, offshore high variability,
offshore low variability regimes). Our results may therefore be crude but
useful estimates of the temporal resolution.</p>
      <p id="d1e1180">We somewhat subjectively define the effective resolution to be the
wavelength above which the NSR exceeds 0.5. In other words, it corresponds
to the threshold where the mapping error variance is 2 times smaller than
the observed true signal variance. The methodology used here is similar to
that by Chelton et al. (2019), except that Chelton et al. (2019) consider the
NSR in the spatial domain, whereas we here consider the NSR in the
wavenumber domain. To illustrate and discuss the impact of the choice of the
NSR criterion on the resolution, a sensitivity study is provided in
Appendix B. We demonstrate that the resolution can be <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> %
coarser with NSR <inline-formula><mml:math id="M83" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.25 (SNR <inline-formula><mml:math id="M84" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 4) and <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> % coarser with
a more conservative NSR criterion (e.g., SNR <inline-formula><mml:math id="M86" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 10, as recommended by Chelton et al., 2019). It is worth mentioning that various approaches may exist to estimate the resolution (e.g., spectral magnitude ratio, filter transfer function). All measures of resolution have their advantages and drawbacks. We discuss in Appendix A the impact of using these different approaches in the estimation of the effective resolution.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e1226">Effective spatial resolution, in kilometers, of the DUACS-DT2018 maps for <bold>(a)</bold> the Global Ocean product <bold>(b)</bold> the Mediterranean Sea and the Black Sea products; units in kilometers.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f02.jpg"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
</sec>
<?pagebreak page1094?><sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Effective resolutions of the DUACS-DT2018 maps</title>
      <p id="d1e1259">The effective spatial resolution of the DUACS-DT2018 global maps is shown in
Fig. 2a. Resolution was computed for maps constructed with three
altimeters (CryoSat-2, HY-2, Jason-2) over the period 12 April 2014–31 December 2015 and Saral/AltiKa data were used as an independent dataset. We believe that this
assessment of the spatial resolution based on maps constructed with three
altimeter missions may be considered a reasonable averaged estimate since
about three altimeter missions are used in the merging for the CMEMS
products 70 % of the time over the period 1 January 1993–15 May 2017. The resolution ranges from <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> km wavelength at high latitudes to <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">800</mml:mn></mml:mrow></mml:math></inline-formula> km wavelength near the Equator, with a mean resolution at midlatitude near 200 km. Considering that eddy radius characteristic can be estimated as 20 %–25 % of the wavelength (Chelton et al., 2011, 2019), this means that <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> km radius structures are properly resolved in the maps at high latitudes, <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> km radius structures are resolved in the equatorial band and <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> km radius structures are resolved at midlatitudes. The effective spatial resolution of the DUACS-DT2018 Mediterranean Sea maps ranges from 90 to 160 km wavelength
(Fig. 2b). The averaged resolution is <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">130</mml:mn></mml:mrow></mml:math></inline-formula> km<?pagebreak page1095?> wavelength over the basin. The effective spatial resolution of the DUACS-DT2018 Black Sea maps ranges from 100 to 150 km wavelength and the averaged resolution is
<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">130</mml:mn></mml:mrow></mml:math></inline-formula> km wavelength over the basin (Fig. 2b).</p>
      <p id="d1e1333">The effective temporal resolution of the DUACS-DT2018 maps ranges from 2 to
140 d (Fig. 3). The temporal resolution is heterogeneously
distributed over the global ocean, particularly in the intertropical band
where a wide range of scales is found, linked to the mixture of continental
tide gauges and island tide gauges, with the latter being more
representative of open-ocean conditions. At mid-to-high latitudes the
zonally averaged temporal scales are between 14 and 45 d,
coherent with the temporal correlation scales applied in the mapping
process. The globally averaged effective temporal resolution is estimated to be
<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">34</mml:mn></mml:mrow></mml:math></inline-formula> d.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e1348">Effective temporal resolution in days of the DUACS-DT2018 maps. Unit in days.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f03.jpg"/>

        </fig>

      <p id="d1e1358">The globally averaged resolutions of about 200 km by 34 d are
consistent with the resolutions reported by Chelton et al. (2011, 2014) and
Pujol et al. (2016). Using the spectral ratio method (see Appendix B), they found spatial resolution slightly better than 200 km at midlatitude in
the Pacific Ocean.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Evolution of DUACS</title>
      <p id="d1e1369">We here investigate the impact of the DUACS upgrade from 2010 to 2018
to highlight the progress of the DUACS processing. Resolutions were computed
for maps constructed with two altimeters (TOPEX/Poseidon and Jason-1) over
the period 1 January 2003–31 December 2004 and Geosat Follow-On data were used as an independent dataset. To identify the impact of the DUACS upgrade, we computed the relative improvement or deterioration of the effective resolutions (expressed in percentage) for the upgrade DT2010 to DT2014, and DT2014 to DT2018 (Fig. 4). A negative (positive) value means finer (coarser) resolution with the upgrade. The comparison of the DT2010 and DT2014 processing shows finer resolution (improvement <inline-formula><mml:math id="M95" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 2 %) in DT2014 than in DT2010 in the high variability regions, e.g., the Gulf Stream system, the Kuroshio system and the Antarctic Circumpolar Current (ACC) (Fig. 4a). These improvements are associated with updated processing such as improved instrumental and atmospheric correction, tide correction, intercalibration method and smaller correlation scale in the mapping process. Coarser resolutions in DT2014 than in DT2010 are found in the equatorial band and are potentially linked to larger correlation scales applied in this region in the DT2014, as reported by Pujol et al. (2016). Although the DT2018<?pagebreak page1096?> and DT2014 global maps have similar mean effective spatial resolution, regional investigation highlights <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> % to 10 % improved resolution in DT2018 in highly turbulent regions (Fig. 4b), such as the equatorial region, the Gulf Stream system, the Kuroshio system and some regions in the ACC. These improvements are linked to the new mapping standard (optimized selection of the observations in the turbulent region and a priori knowledge of the SLA variance based on a longer period in DT2018). The loss of resolution in the equatorial South Atlantic is not understood yet.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e1391">Gain/loss of effective spatial resolution for <bold>(a)</bold> the Global Ocean product between DT2014 and DT2010, <bold>(b)</bold> the Global Ocean product between DT2018 and DT2014 and <bold>(c)</bold> the Mediterranean Sea product and the Black Sea products between DT2018 and DT2014. Negative values mean that the resolution capability is finer. Note the different color bar scale between global and regional products.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f04.jpg"/>

        </fig>

      <p id="d1e1409">Similar comparison is performed for the Mediterranean and Black Sea regional
products focusing on the upgrade DT2014 to DT2018. Resolutions were computed
for regional DUACS maps constructed with three altimeters (Jason-2,
CryoSat-2, HY-2) over the period 12 April 2014–31 December 2015 and Saral/AltiKa was used as an independent dataset. The resolution capability of the Mediterranean Sea maps is slightly finer (<inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> %) in DT2018 than in DT2014 (Fig. 4c). The largest improvements (<inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> %) are found in the western Mediterranean basin. The resolution in DT2018 is slightly coarser in the closed seas (Adriatic Sea and Aegean Sea). In these regions, the limited number of along-track data restricts a reliable interpretation of the spectral signal (see Fig. A1). The resolution capability of the Black Sea maps is on average slightly finer (<inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> %) in DT2018 than in DT2014, although a deterioration is found in the central part of the basin, which is also linked to a reduced number of spectral computations (Fig. 4c).</p>
      <p id="d1e1443">The DUACS-DT2018 and the DUACS-DT2014 maps have mean effective temporal
resolutions of <inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">34</mml:mn></mml:mrow></mml:math></inline-formula> d and 37 d, respectively. The differences can be locally larger than 15 %, near 30<inline-formula><mml:math id="M101" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> along the Japanese coast (<inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> d gain), as shown in Fig. 5. In these regions, the temporal resolution in the DUACS-DT2018 is finer than in DUACS-DT2014. These regions also coincide with the largest increased correlation score in the DUACS-DT2018 between SLA time series from maps and from independent tide gauge sensors (Taburet et al., 2019). These coastal improvements are linked to the new altimeter standards in coastal regions in DT2018 (Taburet et al., 2019).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e1477">Gain/loss of effective temporal resolution between DT2018 and DT2014. Negative values mean that the resolution capability is better in DT2018 than DT2014.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f05.jpg"/>

          <?xmltex \hack{\vspace*{10mm}}?>
        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Impact of altimeter constellation on the effective spatial resolution</title>
      <p id="d1e1496">Since the number of altimeter data processed by DUACS varies with
time (according to the availability of satellites and the data quality), we
investigated the impact of the constellation on the effective spatial
resolution. Figure 6 illustrates the impact of the number of altimeters (two or three missions) used in the mapping on the effective spatial resolution. We
verify, with our diagnostic, modest increases of resolving capabilities in
the DUACS maps with increasing number of altimeters and found a globally
averaged gain of resolution of <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> % from maps constructed
with three altimeters compared with two altimeters. The resolution
improvements may be considered modest. The reason is that the same
covariance parameters are used in the optimal interpolation (OI) procedure
regardless of how many altimeters are available. These OI parameters exert
very strong constraints on the filter transfer function of the OI procedure.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e1511">Impact of the satellite constellation on the effective resolution – ratio of effective resolution of <bold>(a)</bold> maps constructed with C2-H2-J2 vs. C2-J2 and <bold>(b)</bold> maps constructed with C2-H2-J2 vs. H2-J2.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f06.jpg"/>

          <?xmltex \hack{\vspace*{10mm}}?>
        </fig>

      <p id="d1e1528">Regional gains of resolution can be larger than 10 %. Additionally, it is
possible to identify the improved resolving capability when a new mission is
introduced into DUACS: for example, Fig. 6a illustrates the
improved resolving capability when mission HY-2 is introduced into the
mapping, Fig. 6b illustrates the improved resolving capability when
mission CryoSat-2 is introduced in the mapping. It is shown that the major
contribution of the HY-2 mission in the mapping is in the high variability
regions (Gulf Stream, Kuroshio, Agulhas systems) while CryoSat-2 contributes
in the mid-to-high-latitude regions. On the global scale, the distribution
of the effective spatial resolution is shifted toward shorter scales when
the number of missions used in the merging increases (Fig. 7) or when
recent altimeters are used in<?pagebreak page1097?> the interpolation (e.g., compare the
resolution maps from DT2018 constructed with historical Jason-1/Envisat
vs. the maps from DT2018 constructed with currently operational missions
Jason2/HY-2 or Jason-2/CryoSat2).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e1534">Distribution of the effective spatial resolution for various altimeter merging configuration.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f07.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Discussion and conclusions</title>
      <?pagebreak page1099?><p id="d1e1552">The present study investigates the resolving capability of the DUACS
delayed-time gridded products (Global, Mediterranean Sea and Black Sea)
delivered through the CMEMS catalogue. The key results are summarized in
Table 1. Our method is based on the noise-to-signal spectral ratio to
estimate the resolution. While along-track altimeter data resolve wavelength
scales on the order of a few tens of kilometers (Dussurget et al., 2011; Dufau
et al., 2016), we found that the merging of these along-track data into
continuous maps in time and space leads to properly resolved structures with
a wavelength scale of 100 km (a feature radius scale of <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> km) at high latitudes to 800 km (a feature radius scale of <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> km) near the Equator in the global gridded product and with a temporal scale of about 34 d. The same analysis applied to the regional Mediterranean Sea and Black Sea products showed resolving capability of structure with feature radius resolution of <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> km, which corresponds to <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> points grid spacing.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e1598">Summary of the DUACS products spatial and temporal resolutions. (1) Not estimated due to the limited amount of tide gauges in the Mediterranean Sea and Black Sea.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.91}[.91]?><oasis:tgroup cols="6">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="center"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry rowsep="1" namest="col2" nameend="col3" align="center">Spatial feature </oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry rowsep="1" namest="col5" nameend="col6" align="center">Temporal feature </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Product</oasis:entry>
         <oasis:entry colname="col2">Effective</oasis:entry>
         <oasis:entry colname="col3">Grid</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">Effective</oasis:entry>
         <oasis:entry colname="col6">Grid</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">resolution</oasis:entry>
         <oasis:entry colname="col3">spacing</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">resolution</oasis:entry>
         <oasis:entry colname="col6">spacing</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Global</oasis:entry>
         <oasis:entry colname="col2">100 to 800 km</oasis:entry>
         <oasis:entry colname="col3">4 to 30 km</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">34</mml:mn></mml:mrow></mml:math></inline-formula> d</oasis:entry>
         <oasis:entry colname="col6">1 d</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Med. Sea</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">130</mml:mn></mml:mrow></mml:math></inline-formula> km</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> km</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">(1)</oasis:entry>
         <oasis:entry colname="col6">1 d</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Black Sea</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">130</mml:mn></mml:mrow></mml:math></inline-formula> km</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> km</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">(1)</oasis:entry>
         <oasis:entry colname="col6">1 d</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <p id="d1e1787">These results are consistent with previous investigations. Based on a
spectral ratio approach (cf. Appendix B), Chelton et al. (2011) estimated a
wavelength resolution of <inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> km for DT2010 and Chelton et al. (2014) estimated a wavelength resolution of <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">180</mml:mn></mml:mrow></mml:math></inline-formula> km for DT2014 in the midlatitude Pacific Ocean. Our analysis, based on the DT2018 global maps, suggests a wavelength resolution of <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> km at midlatitudes. As illustrated in Fig. 8, we verified that our estimation of the zonally averaged feature radius resolution of the mesoscale structures that can be properly mapped is smaller than the eddy scales computed by Chelton et al. (2011). The eddy length scales range from <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> km at high latitudes to <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">180</mml:mn></mml:mrow></mml:math></inline-formula> km near the Equator. The effective resolution is <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.6</mml:mn></mml:mrow></mml:math></inline-formula> times smaller than the eddy length scale. Additionally, we confirm that the minimum 4-week lifetime criteria used by Chelton et al. (2011) to identify and follow eddies seems to be compatible with the 34 d resolution capability. Note that our timescale estimation is based mainly on coastal locations and might not be representative of all oceanic regimes.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e1854">Zonally averaged eddy scale (as in Chelton et al., 2011; and computed from the DUACS-DT2018 two satellites maps) and feature radius resolution of the mesoscale structures that can be properly mapped in DUACS (i.e., derived as 0.25 <inline-formula><mml:math id="M119" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> effective resolution). Units in kilometers.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f08.png"/>

      </fig>

      <p id="d1e1870">The comparison of the DUACS-DT2018 reprocessing with former DUACS
reprocessing (DT2010 and DT2014) reveals that finer structures are mapped in
the global and regional Mediterranean Sea DT2018 products. For the Black Sea
product, the interpretation is more complex due to the small dimension of
the basin and the limited amount of spectral computation. Globally, we found
that the largest improvements reach 20 % and are mainly in high
variability regions, associated with the new mapping standard (e.g.,
optimized selection of the along-track data, new a priori knowledge of the
signal variance based on 25 years of altimetry data, updated correlation
scales for the regional<?pagebreak page1100?> Mediterranean Sea product) and new altimeter
standards (e.g., instrumental and atmospheric corrections, tide corrections,
intercalibration method). The improvement patterns between DT2014 and
DT2010 global maps are similar to those found by Pujol et al. (2016) using statistical comparison between maps and independent along-track, and drifter, datasets. The improvement patterns between DT2018 and DT2014 global maps coincide with those found by Taburet el al. (2019) for the validation of the DT2018 products. Using statistical comparison between maps and independent along-track altimeter data, Taburet et al. (2019) also found improvement (<inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> %–4 %) of the mapped mesoscale structures in
the high variability region and in the western Mediterranean Sea basin. Note
that, at global scale, Taburet et al. (2019) diagnosed the largest
improvements between DT2018 and DT2014 in the coastal regions which are
partially edited (along 100 km coastal band) in the processing for estimating the spatial scale in this study, but they are detected with the temporal scale analysis showing shorter timescale in the DT2018 compared with DT2014.</p>
      <p id="d1e1883">Several studies showed that at least two altimeters are required to
accurately map the SSH mesoscale structures (Le Traon and Dibarboure, 1999;
Ducet et al., 2000; Pujol and Larnicol, 2005; Dibarboure et al., 2011; Chelton et al., 2007, 2011) and up to four altimeters are required for near-real-time products (Pascual et al., 2006) because only past observations are available for the mapping. This reduced number of observations has an impact on the estimation of the sea surface height. The present study reinforces these findings, showing that the resolution capability increased <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> %–20 % at regional scale from the merging of data from two to three altimeters.</p>
      <p id="d1e1896">It is worth noting that we probably underestimate the resolution capability
of the maps since we are estimating the spatial effective resolution of
degraded maps to keep an independent dataset aside. The resolution might
hence be somewhat finer in the distributed CMEMS products. Although the
satellite constellation ranges from 1 to 5 altimeter(s) between 1 January 1993 and 15 May 2017, we believe that our estimation of the spatial resolution based on maps constructed with three altimeter missions may be considered a reasonable averaged estimate since about three altimeter missions are used in the merging for the CMEMS products 70 % of the time over the period 1 January 1993–15 May 2017. We can expect <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> % finer resolution over the period where more than four altimeters are available (i.e., recent period). Likewise, we can expect on average 5 % coarser resolution when only two altimeters are available.</p>
      <p id="d1e1909"><?xmltex \hack{\newpage}?>To conclude, the number and the quality of altimeters simultaneously
operational, the along-track configuration and sampling pattern, the weight
given to the altimeter data in the mapping procedure, and the choice of
threshold SNR are key factors controlling the resolution capability of the
DUACS gridded products. One may expect that in permitting to observe finer
mesoscale or sub-mesoscale structures (Dufau et al., 2016; Pujol et al., 2012), future instrumental systems based on large-swath altimeters (such as Surface
Ocean and Water Topography – SWOT) combined with new mapping techniques based
on dynamic interpolation (Ubelmann et al., 2016) will push the
resolution of maps toward new limits.</p>
</sec>

      
      </body>
    <back><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d1e1918">The DUACS source code is not publicly available. The code for the spectral analysis is released under GNU General Public License v3.0 and is available at <uri>https://github.com/mballaro/scuba</uri> (last access: 16 August 2019). DUACS all satellite gridded data and along-track data are available through the CMEMS website: <uri>http://marine.copernicus.eu/</uri> (last access: 16 August 2019). Specific maps used in our study are based on merging of three or two satellites and are available on request by contacting Maxime Ballarotta (mballarotta@groupcls.com).</p>
  </notes><?xmltex \hack{\clearpage}?><app-group>

<?pagebreak page1101?><app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>Other approach to estimate the resolution</title>
<sec id="App1.Ch1.S1.SS1">
  <label>A1</label><title>Spectral magnitude ratio</title>
      <p id="d1e1945">Chelton et al. (2011, 2014) estimated the resolution of the DUACS-DT2014
maps based on the calculation of the spectral magnitude ratio between the
reference Stammer (1997) along-track spectrum and gridded SSH spectra.
Similarly, we here estimate the resolution based on the spectral ratio
between independent along-track and gridded SSH signals (Eq. A1). It is
defined as follows:
            <disp-formula id="App1.Ch1.S1.E3" content-type="numbered"><label>A1</label><mml:math id="M123" display="block"><mml:mrow><mml:mi mathvariant="normal">SR</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">map</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> denotes the power spectral
density of the independent SSH along-track, <inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">map</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> denotes the power spectral density of the SSH map interpolated onto the independent along-track segment, SR the spectral ratio and <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> the wavelength. The resolution is given by the wavelength <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> where the spectral ratio is equal to 0.5 and is based on the conventional notion of a filter being characterized by its half-power filter cutoff wavelength (Chelton et al., 2011). To differentiate it from the effective resolution, we named it useful resolution: useful for verifying the available and realistic amount of energy at a specific wavelength between two signals without considering their phase (e.g., useful for model sensitivity study).</p>
      <p id="d1e2057">Chelton et al. (2011, 2014) estimated the resolution of the DUACS-DT2010 and
DUACS-DT2014 as the wavenumber at which the power is a factor of 2 smaller
than the Stammer (1997) spectrum. From their analysis, they estimated
a spatial resolution of <inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M129" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> for the DUACS-DT2010 and <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.7</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M131" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> for the DUACS-2014. Chelton et al. (2014) found essentially the same resolution between maps constructed with two or four satellites.</p>
      <p id="d1e2096">The resolution estimated with the SR method is shown in Fig. A2a and the
difference between the effective and useful resolutions is shown in Fig. A2b. The useful resolution of the DUACS-DT2018 maps ranges from 100 km at
high latitude to 500 km near the Equator. The ratio of effective to useful
resolution suggests somewhat finer resolution in the intertropical band
using the SR approach and somewhat finer resolution at high latitude with the
NSR approach. In other words, the amplitude of the mapped SSH spectral
content is better in the intertropical band than the phase, whereas it is
the opposite at high latitude. This feature highlights the difficulty to
properly map propagating equatorial waves in DUACS. The two
methods are equivalent at midlatitudes.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="App1.Ch1.S1.SS2">
  <label>A2</label><title>Transfer function</title>
      <p id="d1e2108">The transfer function (<inline-formula><mml:math id="M132" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula>) measures the filtering properties of a system (Eq. A2). It is defined as follows:
            <disp-formula id="App1.Ch1.S1.E4" content-type="numbered"><label>A2</label><mml:math id="M133" display="block"><mml:mrow><mml:mi>H</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">CS</mml:mi><mml:mrow><mml:mi mathvariant="normal">obs</mml:mi><mml:mtext>-</mml:mtext><mml:mi mathvariant="normal">map</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where CS<inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">obs</mml:mi><mml:mtext>-</mml:mtext><mml:mi mathvariant="normal">map</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the cross-spectral density between the along-track data and the map interpolated onto the along-track segment and <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the power spectral density of the along-track. Note that in this case, the along-track data are considered nonindependent (i.e., they are used in the mapping system). The resolution is given by the wavelength <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
where <inline-formula><mml:math id="M137" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> is equal to 0.5. It is the same definition used by Schlax and Chelton (1992) to estimate the resolution capability of an arbitrarily sampled dataset.</p>
      <p id="d1e2233">The resolution estimated with the transfer function method is shown in
Fig. A3a and the difference between the effective resolution and the
transfer function resolution is shown in Fig. A3b. The transfer function
resolution of the DUACS-DT2018 maps ranges from 100 km at high latitude to
400 km near the Equator. The difference between effective resolution vs. transfer function resolution suggests somewhat finer resolution using the
transfer function. This is directly linked to the fact that the along-track
data are here nonindependent. The assessment is undertaken below the track that
is used in the filtering system. This diagnostic gives the filtering
property of the system but suffers from nonindependency of the
along-track dataset. The resolution may be different off-track.</p>
      <p id="d1e2236">These methods share the same number of spectrum calculation and number of
segments used in the calculation (see Fig. A1) and each method has
advantages and drawbacks. The spectral magnitude ratio compares the
amplitude of the signals and the transfer function estimates the filtering
properties from assimilated along-track data. The functions NSR(<inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, SR<inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:mi>H</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> are shown for location (45<inline-formula><mml:math id="M141" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 330<inline-formula><mml:math id="M142" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) in
Fig. A4. At this location, each function has a transition between 100 and
200 km wavelength, separating the high mapping error regime for
wavelength <inline-formula><mml:math id="M143" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 100 km to the low mapping error for wavelength <inline-formula><mml:math id="M144" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 200 km (Fig. A4a), separating the high amplitude error regime for wavelength <inline-formula><mml:math id="M145" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 100 km to the low amplitude error for
wavelength <inline-formula><mml:math id="M146" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 200 km (Fig. A4b), and separating the filter regimes (Fig. A4c).</p><?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F9"><?xmltex \currentcnt{A1}?><label>Figure A1</label><caption><p id="d1e2334">Number of segments used in the spectral computation for <bold>(a)</bold> the global product and <bold>(b)</bold> the regional Mediterranean and Black Sea products.</p></caption>
          <?xmltex \hack{\hsize\textwidth}?>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f09.jpg"/>

        </fig>

<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F10"><?xmltex \currentcnt{A2}?><label>Figure A2</label><caption><p id="d1e2354"><bold>(a)</bold> DUACS-DT2018 useful resolution derived from spectral ratio (SR) approach and <bold>(b)</bold> ratio of effective to useful resolution for the DT2018 maps. Blue means finer resolution with NSR.</p></caption>
          <?xmltex \hack{\hsize\textwidth}?>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f10.jpg"/>

        </fig>

<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F11"><?xmltex \currentcnt{A3}?><label>Figure A3</label><caption><p id="d1e2373"><bold>(a)</bold> DUACS-DT2018 resolution derived from the transfer function approach and <bold>(b)</bold> ratio of effective to transfer function resolution for the DT2018 maps. Blue means finer resolution with NSR.</p></caption>
          <?xmltex \hack{\hsize\textwidth}?>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f11.jpg"/>

        </fig>

<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F12"><?xmltex \currentcnt{A4}?><label>Figure A4</label><caption><p id="d1e2393">Illustration of the various spectral functions used to estimate the resolution at 45<inline-formula><mml:math id="M147" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 330<inline-formula><mml:math id="M148" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E: <bold>(a)</bold> with NSR method, <bold>(b)</bold> with SR method and <bold>(c)</bold> with the transfer function (<inline-formula><mml:math id="M149" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula>).</p></caption>
          <?xmltex \hack{\hsize\textwidth}?>
          <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f12.png"/>

        </fig>

<?xmltex \hack{\clearpage}?>
</sec>
</app>

<?pagebreak page1106?><app id="App1.Ch1.S2">
  <?xmltex \currentcnt{B}?><label>Appendix B</label><title>Sensitivity of the noise-to-signal ratio (NSR) criterion</title>
      <p id="d1e2450">We here investigate and discuss the impact of the NSR criterion on the
estimation of the effective resolution. NSR criterion is used to define the
resolution limit of the map. In the present study, we choose the NSR <inline-formula><mml:math id="M150" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.5 criterion to define the resolution limit. This value may be considered too generous; therefore, we present below the effective resolution for three cases, motivated by the analysis performed in the spatial domain by Chelton et al. (2019):
<list list-type="bullet"><list-item>
      <p id="d1e2462">criterion of NSR <inline-formula><mml:math id="M151" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.5,</p></list-item><list-item>
      <p id="d1e2473">criterion of NSR <inline-formula><mml:math id="M152" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.25,</p></list-item><list-item>
      <p id="d1e2484">criterion of NSR <inline-formula><mml:math id="M153" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.1.</p></list-item></list>
Figure B1a represents the effective resolution using NSR <inline-formula><mml:math id="M154" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.5 (SNR <inline-formula><mml:math id="M155" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2) criterion, Fig. B1b using NSR <inline-formula><mml:math id="M156" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.25 (SNR <inline-formula><mml:math id="M157" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 4) criterion and Fig. B1c NSR <inline-formula><mml:math id="M158" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.1 (SNR <inline-formula><mml:math id="M159" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 10). For each panel the resolution becomes finer poleward. The white areas correspond to the regions where the NSR threshold criterion is not achieved. These areas become larger in the intertropical region as well as at high latitudes when the NSR criterion decreases. For NSR <inline-formula><mml:math id="M160" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.1, the resolution in the intertropical band cannot be computed with the method since the NSR is above 0.1 for all scales. To further illustrate this, we show an example of NSR at one specific point (lat <inline-formula><mml:math id="M161" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 16<inline-formula><mml:math id="M162" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, long <inline-formula><mml:math id="M163" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 346<inline-formula><mml:math id="M164" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) in Fig. B2. The analysis shows that the NSR is greater than 0.3 (i.e., SNR <inline-formula><mml:math id="M165" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 3) in this location. This large-scale low coherency between maps and along-track may be linked to the misrepresentation of the large-scale and rapid equatorial waves (e.g., equatorial gravity waves) in the mapping process, which are filtered in the mapping process.</p>
      <p id="d1e2585"><?xmltex \hack{\newpage}?>Despite the areas of missing values in Fig. B1b and c, we quantify the difference in effective resolution between criterion NSR <inline-formula><mml:math id="M166" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.4 and
NSR <inline-formula><mml:math id="M167" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.25 (Fig. B3) and NSR <inline-formula><mml:math id="M168" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.5 and NSR <inline-formula><mml:math id="M169" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.1. The difference between effective resolution computed with NSR <inline-formula><mml:math id="M170" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.5 vs. NSR <inline-formula><mml:math id="M171" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.25 is <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> % (<inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> km) at midlatitude and <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mo>=</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> % (400 km) in the intertropical band. The difference between effective resolution computed with NSR <inline-formula><mml:math id="M175" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.5 vs. NSR <inline-formula><mml:math id="M176" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.1 is <inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> % (<inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> km) at midlatitude and <inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> % in the intertropical band.</p>
      <p id="d1e2709">In conclusion, we here demonstrate that the choice of the NSR criterion has
an impact on the estimation of the resolution. Setting a more conservative
criterion of NSR <inline-formula><mml:math id="M180" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.25 leads to <inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> % coarser effective resolution. The strongly conservative criterion NSR <inline-formula><mml:math id="M182" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.1 also reveals one of the major caveats in the DUACS maps processing: the poor representation of the large-scale and rapid equatorial circulation. This issue should be
addressed in a future version of DUACS maps.</p><?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S2.F13"><?xmltex \currentcnt{B1}?><label>Figure B1</label><caption><p id="d1e2739">Effective resolution computed for three different SNR criteria: <bold>(a)</bold> SNR <inline-formula><mml:math id="M183" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2, <bold>(b)</bold> SNR <inline-formula><mml:math id="M184" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 4 and <bold>(c)</bold> SNR <inline-formula><mml:math id="M185" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 10. The white areas correspond to the regions where the SNR threshold criterion is not achieved.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f13.jpg"/>

      </fig>

<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.S2.F14"><?xmltex \currentcnt{B2}?><label>Figure B2</label><caption><p id="d1e2784">Ratio of NSR at longitude 346<inline-formula><mml:math id="M186" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E and latitude 16<inline-formula><mml:math id="M187" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S. We illustrate that the ratio at this location is always above <inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula> and so the resolution cannot be computed for SNR criterion <inline-formula><mml:math id="M189" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 4 (i.e., NSR <inline-formula><mml:math id="M190" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.25).</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f14.png"/>

      </fig>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S2.F15"><?xmltex \currentcnt{B3}?><label>Figure B3</label><caption><p id="d1e2839">Ratio of effective resolution computed with <bold>(a)</bold> SNR <inline-formula><mml:math id="M191" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2 vs. SNR <inline-formula><mml:math id="M192" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 4 criterion and <bold>(b)</bold> SNR <inline-formula><mml:math id="M193" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2 vs. SNR <inline-formula><mml:math id="M194" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 10 criterion. Blue means finer resolution with SNR <inline-formula><mml:math id="M195" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2. The white areas correspond to the regions where the SNR threshold criterion is not achieved.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://os.copernicus.org/articles/15/1091/2019/os-15-1091-2019-f15.jpg"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2898">CU initiated the study. MB and CU designed the study and implemented the Scuba tools. GT, MIP, FF, JFL, YF, AD, DC, GD and NP helped in the design and discussion of the results. MB wrote the paper with contributions from all coauthors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2904">The authors declare that they have no conflict of interest.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e2910">This article is part of the special issue “The Copernicus Marine Environment Monitoring Service (CMEMS): scientific advances”. It is not associated with a conference.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2916">This work is a contribution to the CMEMS R &amp; D activities, the CNES-SALP
project and the BOOST-SWOT project. We would like to thank Lee Lueng Fu for his suggestions on the paper, Tom Farrar for his detailed and inspiring
review, and one anonymous referee. All their comments significantly added
value to this paper.</p></ack><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2921">This paper was edited by Emil Stanev and reviewed by Tom Farrar, Fu Lee Lueng, and one anonymous referee.</p>
  </notes><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e2927">This research has been supported by the ANR (grant number ANR-17-CE01-0009-01).</p>
  </notes><ref-list>
    <title>References</title>

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    <!--<article-title-html>On the resolutions of ocean altimetry maps</article-title-html>
<abstract-html><p>The Data Unification and Altimeter Combination System (DUACS) produces sea level global and regional
maps that serve oceanographic applications, climate forecasting centers,
and geophysics and biology communities. These maps are generated using an
optimal interpolation method applied to altimeter observations. They are
provided on a global 1∕4°&thinsp; × &thinsp;1∕4° (longitude&thinsp; × &thinsp;latitude) and daily grid resolution framework
(1∕8°&thinsp; × &thinsp;1∕8° longitude&thinsp; × &thinsp;latitude grid for the regional products) through the Copernicus Marine Environment Monitoring Service (CMEMS). Yet, the dynamical content of these maps does not have full 1∕4° spatial and 1&thinsp;d temporal resolutions due to the
filtering properties of the optimal interpolation. In the present study, we
estimate the effective spatial and temporal resolutions of the newly
reprocessed delayed-time DUACS maps (a.k.a. DUACS-DT2018). Our approach is
based on the ratio between the spectral content of the mapping error and the
spectral content of independent true signals (along-track and tide gauge
observations), also known as the noise-to-signal ratio. We found that the
spatial resolution of the DUACS-DT2018 global maps based on sampling by
three altimeters simultaneously ranges from  ∼ 100&thinsp;km wavelength
at high latitude to  ∼ 800&thinsp;km wavelength in the equatorial band
and the mean temporal resolution is  ∼ 34&thinsp;d. The mean
effective spatial resolution at midlatitude is estimated to be  ∼ 200&thinsp;km. The mean effective spatial resolution is  ∼ 130&thinsp;km for
the regional Mediterranean Sea and for the regional Black Sea products. An
intercomparison with previous DUACS reprocessing systems (a.k.a., DUACS-DT2010
and DUACS-DT2014) highlights the progress of the system over the past 8 years, in particular a gain of resolution in highly turbulent regions. The same diagnostic applied to maps constructed with two altimeters and maps with three altimeters confirms a modest increase in resolving capabilities and accuracies in the DUACS maps with the number of missions.</p></abstract-html>
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Description, First Tandem Results and Impact on Processing and Products, Mar. Geod., 34, 214–241, <a href="https://doi.org/10.1080/01490419.2011.584826" target="_blank">https://doi.org/10.1080/01490419.2011.584826</a>, 2011.
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Le Traon, P. Y. and Dibarboure, G.: Mesoscale mapping capabilities from multiple altimeter missions, J. Atmos. Ocean. Tech., 16, 1208–1223, 1999.
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<ref-html id="bib1.bib12"><label>12</label><mixed-citation>
Le Traon, P. Y., Nadal, F., and Ducet, N.: An improved mapping method of
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</mixed-citation></ref-html>
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Pujol, M. I. and Larnicol, G.: Mediterranean Sea eddy kinetic energy
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</mixed-citation></ref-html>
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Pujol, M.-I., Dibarboure, G., Le Traon, P.-Y., and Klin, P.: Using high-resolution altimetry to observe mesoscale signals, J. Atmos. Ocean. Tech., 29, 140–141, <a href="https://doi.org/10.1175/JTECH-D-12-00032.1" target="_blank">https://doi.org/10.1175/JTECH-D-12-00032.1</a>, 2012.
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Pujol, M.-I., Faugère, Y., Taburet, G., Dupuy, S., Pelloquin, C., Ablain, M., and Picot, N.: DUACS DT2014: the new multi-mission altimeter data set reprocessed over 20 years, Ocean Sci., 12, 1067–1090, <a href="https://doi.org/10.5194/os-12-1067-2016" target="_blank">https://doi.org/10.5194/os-12-1067-2016</a>, 2016.
</mixed-citation></ref-html>
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Schlax, M. G. and Chelton, D. B.: Frequency domain diagnostics for linear smoothers, J. Am. Stat. Assoc., 87, 1070–1081, 1992.
</mixed-citation></ref-html>
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Stammer, D.: Global characteristics of ocean variability estimated from
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Taburet, G., Sanchez-Roman, A., Ballarotta, M., Pujol, M.-I., Legeais, J.-F., Fournier, F., Faugere, Y., and Dibarboure, G.: DUACS DT-2018: 25 years of reprocessed sea level altimeter products, Ocean Sci. Discuss.,
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</mixed-citation></ref-html>--></article>
