O+ escape in the polar ion exosphere of Mars
β Scribed by S.A. Haider
- Publisher
- Elsevier Science
- Year
- 1995
- Tongue
- English
- Weight
- 645 KB
- Volume
- 16
- Category
- Article
- ISSN
- 0273-1177
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
As a part of a global effort, the dynamics of energetic particles flowing through the martian upper atmosphere is studied. Most of the production of hot atomic oxygen occurs deep in the day-side thermosphere of Mars, where dissociative recombination (DR) of O ΓΎ 2 ion is the dominant source. The stud
A HovmΓΆller diagram analysis of the dust optical depth measured by the Mars Global Surveyor Thermal Emission Spectrometer shows the occurrence of quasi-periodic westwardly-propagating disturbances with timescales of 10-20 sols during summer in the south polar region of Mars. Dust clouds emerge repea
The perennial north polar H 2 O ice cap of Mars is investigated with the dynamic/thermodynamic ice-sheet model SICOPOLIS. Computational results for flow velocities, ice temperatures, and surface accumulation/ablation rates are presented for the steady state with present conditions as well as for tra