Water vapor saturation state on Mars from ACS-NIR/TGO occultations from MY34 to MY36

Published: 14 October 2022| Version 1 | DOI: 10.17632/6xrn9v4dc5.1
Contributor:
Anna Fedorova

Description

Dataset for the publication "A two-Martian year survey of the water vapor saturation state on Mars based on ACS NIR/TGO occultations" by Fedorova et al. Includes a list of orbits, and H2O mixing ratio in ppmv, saturation ratio (S), temperature (T) in K and aerosol extinction at 1.4 mum in km-1 from ACS NIR/TGO solar occultation observations from Ls=163 of MY34 to Ls=170 of MY35. Data contain folders with the list of orbits and H2O volume mixing ratio, S, T and extinction for each orbit of TGO where ACS-NIR had measurements. H2O and S data files are named "orbXXXXXX_NY_H2O_S_ACSNIR.txt", temperature data files are named "orbXXXXXX_NY_temperature_ACSNIR.txt", extinction data files are named "orbXXXXXX_NY_aerosol_extinction_ACSNIR.txt", where XXXXXX is the decimal orbit number, Y is the occultation number in orbit.

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Categories

Saturation, Planetary Atmosphere, Mars, Water Vapor

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