Articles | Volume 17, issue 17
https://doi.org/10.5194/amt-17-5161-2024
https://doi.org/10.5194/amt-17-5161-2024
Research article
 | 
05 Sep 2024
Research article |  | 05 Sep 2024

How well can brightness temperature differences of spaceborne imagers help to detect cloud phase? A sensitivity analysis regarding cloud phase and related cloud properties

Johanna Mayer, Bernhard Mayer, Luca Bugliaro, Ralf Meerkötter, and Christiane Voigt

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Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • CC1: 'Comment on egusphere-2024-540', Andrew Heidinger, 22 Mar 2024
  • RC1: 'Comment on egusphere-2024-540', Anonymous Referee #1, 01 Apr 2024
  • RC2: 'Comment on egusphere-2024-540', Anonymous Referee #2, 30 Apr 2024

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Johanna Mayer on behalf of the Authors (21 May 2024)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (23 May 2024) by Andrew Sayer
RR by Anonymous Referee #2 (27 Jun 2024)
ED: Publish as is (27 Jun 2024) by Andrew Sayer
AR by Johanna Mayer on behalf of the Authors (28 Jun 2024)
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Short summary
This study uses radiative transfer calculations to characterize the relation of two satellite channel combinations (namely infrared window brightness temperature differences – BTDs – of SEVIRI) to the thermodynamic cloud phase. A sensitivity analysis reveals the complex interplay of cloud parameters and their contribution to the observed phase dependence of BTDs. This knowledge helps to design optimal cloud-phase retrievals and to understand their potential and limitations.