Water vapor on Mars from SPICAM IR occultations (MY27-34)

Published: 3 June 2021| Version 2 | DOI: 10.17632/vx4gks6bx7.2
Anna Fedorova


Dataset for the publication "Multi-annual monitoring of the water vapor vertical distribution on Mars by SPICAM on Mars Express" by Fedorova et al. Includes a list of orbits, and H2O density in cm-3 and H2O mixing ratio in ppm from SPICAM IR/MEX solar occultation observations for 8 Martian years from 27 to 34. Data contain two folders with the list of orbits and H2O density and volume mixing ratio for each orbit. H2O data files are named "orbXXXXXAY_H2O_vmr(density).txt", where XXXXX is the decimal orbit number, Y is the occultation number in orbit.



Planetary Atmosphere, Occultation, Dust Storm, Mars, Water Vapor