Solar Cycle Variations of the Hydrogen E
โ
V.A. Krasnopolsyky
๐
Article
๐
1993
๐
Elsevier Science
๐
English
โ 480 KB
A one-dimensional photochemical model of the Martian atmosphere has been developed to study variations in the atmospheric composition with solar activity. The low sensitivity of \(\mathrm{O}\) and \(\mathrm{CO}\) number densities near the ionospheric peak to solar activity suggests that eddy mixing