Articles | Volume 17, issue 2
https://doi.org/10.5194/os-17-455-2021
https://doi.org/10.5194/os-17-455-2021
Technical note
 | 
11 Mar 2021
Technical note |  | 11 Mar 2021

Technical note: A sensitivity analysis from 1 to 40 GHz for observing the Arctic Ocean with the Copernicus Imaging Microwave Radiometer

Lise Kilic, Catherine Prigent, Carlos Jimenez, and Craig Donlon

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Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
AR by Lise Kilic on behalf of the Authors (14 Jan 2021)  Manuscript 
ED: Reconsider after major revisions (15 Jan 2021) by John M. Huthnance
AR by Lise Kilic on behalf of the Authors (19 Jan 2021)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (20 Jan 2021) by John M. Huthnance
RR by Anonymous Referee #1 (26 Jan 2021)
RR by Anonymous Referee #3 (28 Jan 2021)
ED: Publish as is (29 Jan 2021) by John M. Huthnance
AR by Lise Kilic on behalf of the Authors (05 Feb 2021)  Manuscript 
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Short summary
The Copernicus Imaging Microwave Radiometer (CIMR) is one of the high-priority satellite missions of the Copernicus program within the European Space Agency. It is designed to respond to the European Union Arctic policy. Its channels, incidence angle, precisions, and spatial resolutions have been selected to observe the Arctic Ocean with the recommendations expressed by the user communities. In this note, we present the sensitivity analysis that has led to the choice of the CIMR channels.