Articles | Volume 13, issue 11
https://doi.org/10.5194/amt-13-6293-2020
https://doi.org/10.5194/amt-13-6293-2020
Research article
 | 
24 Nov 2020
Research article |  | 24 Nov 2020

Correction of a lunar-irradiance model for aerosol optical depth retrieval and comparison with a star photometer

Roberto Román, Ramiro González, Carlos Toledano, África Barreto, Daniel Pérez-Ramírez, Jose A. Benavent-Oltra, Francisco J. Olmo, Victoria E. Cachorro, Lucas Alados-Arboledas, and Ángel M. de Frutos

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AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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AR: Author's response | RR: Referee report | ED: Editor decision
AR by Roberto Román on behalf of the Authors (08 Oct 2020)  Author's response   Manuscript 
ED: Referee Nomination & Report Request started (12 Oct 2020) by Omar Torres
RR by Anonymous Referee #1 (14 Oct 2020)
ED: Publish as is (14 Oct 2020) by Omar Torres
AR by Roberto Román on behalf of the Authors (14 Oct 2020)
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Short summary
Atmospheric-aerosol and gaseous properties can be derived at night-time if the lunar irradiance at the ground is measured. To this end, the knowledge of lunar irradiance at the top of the atmosphere is necessary. This extraterrestrial lunar irradiance is usually calculated by models since it varies with several geometric factors mainly depending on time and location. This paper proposes a correction to the most used lunar-irradiance model to be applied for atmospheric-aerosol characterization.