Evolutionary impact of sputtering of the Martian atmosphere by O+ pickup ions

Geophysical Research Letters

Volumn 19, Issue 21, 1992, Pages 2151-2154

  Luhmann, J G ^a   Johnson, R E ^b   Zhang, M H G ^c  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF VIRGINIA   (United States)

^c Space Research Institute ^*  (Austria)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 84921498107     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/92GL02485     Document Type: Article

References (28)

1. Detectability of Martian carbonates from orbit using thermal neutrons
2. Nitrogen escape from Mars
3. The fast atomic oxygen corona extent of Mars
4. Comment on “Dayside pick‐up oxygen ion precipitation at Venus and Mars,”
5. CO2 Condensation and the climate of early Mars
6. A model of the ion wake of Mars
7. Dayside pickup oxygen ion precipitation at Venus and Mars: Spatial distributions, energy deposition and consequences
8. On the momentum transfer of the solar wind to the Martian topside ionosphere
9. ASPERA/Phobos measurements of the ion outflow from the Martian ionosphere
10. Mars: An evolving atmosphere
11. Photochemistry and evolution of Mars' atmosphere: A Viking perspective
12. Magnetospheric plasma sputtering of lo's atmosphere
13. The early environment and its evolution on Mars: Implications for life
14. Hot oxygen atoms in the upper atmospheres of Venus and Mars
15. Hot hydrogen and oxygen atoms in the upper atmospheres or Venus and Mars
16. Solar wind erosion of the Mars early atmosphere
17. Ejection of atoms and molecules from Io by plasma‐ion impact
18. Thermal history of Mars and the sulfur content of its core
19. A new predictive model for determining solar wind‐terrestrial planet interactions
20. On the problem of the Martian atmosphere dissipation: Phobos 2 TAUS spectrometer results
21. Solar wind sputtering effects in the atmospheres of Mars and Venus
22. The evolution of solar ultraviolet luminosity
23. The ancient oxygen exosphere of Mars: Implications for atmosphere evolution
24. Oxygen ionization rates at Mars and Venus: Relative contributions of impact ionization and charge exchange