Abstract
The ultraviolet dayglow spectrum arising from emission of N 2 in the Mars atmosphere is predicted. The intensities are such that a high-resolution spectrum should readily reveal the presence of N 2 at the abundances suggested by the Viking experiments.
Original language | American English |
---|---|
Journal | Journal of Geophysical Research |
Volume | 82 |
DOIs | |
State | Published - Jan 1 1977 |
Disciplines
- Astrophysics and Astronomy
- Physical Sciences and Mathematics
- Physics