Abstract
Theoretical results of hot carbon densities in the exosphere of Mars are presented. The calculation is a two-step process: First a two-stream transport code is used to solve for the distribution function at the exobase, and then these results are used in a Liouville equation solution above the exobase. It is found that photodissociation of carbon monoxide is the largest source of hot carbon atoms in the upper atmosphere of Mars, larger than dissociative recombination of CO+ and much larger than the creation of hot carbon through collisions with hot oxygen atoms. It is also found that the high solar activity densities are about an order of magnitude larger than those for the low solar activity case.
| Original language | English |
|---|---|
| Article number | 2001JA000007 |
| Pages (from-to) | 21565-21568 |
| Number of pages | 4 |
| Journal | Journal of Geophysical Research: Space Physics |
| Volume | 106 |
| Issue number | A10 |
| Publication status | Published - 2001 Oct 1 |
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All Science Journal Classification (ASJC) codes
- Geophysics
- Forestry
- Oceanography
- Aquatic Science
- Ecology
- Water Science and Technology
- Soil Science
- Geochemistry and Petrology
- Earth-Surface Processes
- Atmospheric Science
- Earth and Planetary Sciences (miscellaneous)
- Space and Planetary Science
- Palaeontology
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Hot carbon densities in the exosphere of Mars. / Nagy, Andrew F.; Liemohn, Michael W.; Fox, J. L.; Kim, Jhoon.
In: Journal of Geophysical Research: Space Physics, Vol. 106, No. A10, 2001JA000007, 01.10.2001, p. 21565-21568.Research output: Contribution to journal › Article
TY - JOUR
T1 - Hot carbon densities in the exosphere of Mars
AU - Nagy, Andrew F.
AU - Liemohn, Michael W.
AU - Fox, J. L.
AU - Kim, Jhoon
PY - 2001/10/1
Y1 - 2001/10/1
N2 - Theoretical results of hot carbon densities in the exosphere of Mars are presented. The calculation is a two-step process: First a two-stream transport code is used to solve for the distribution function at the exobase, and then these results are used in a Liouville equation solution above the exobase. It is found that photodissociation of carbon monoxide is the largest source of hot carbon atoms in the upper atmosphere of Mars, larger than dissociative recombination of CO+ and much larger than the creation of hot carbon through collisions with hot oxygen atoms. It is also found that the high solar activity densities are about an order of magnitude larger than those for the low solar activity case.
AB - Theoretical results of hot carbon densities in the exosphere of Mars are presented. The calculation is a two-step process: First a two-stream transport code is used to solve for the distribution function at the exobase, and then these results are used in a Liouville equation solution above the exobase. It is found that photodissociation of carbon monoxide is the largest source of hot carbon atoms in the upper atmosphere of Mars, larger than dissociative recombination of CO+ and much larger than the creation of hot carbon through collisions with hot oxygen atoms. It is also found that the high solar activity densities are about an order of magnitude larger than those for the low solar activity case.
UR - http://www.scopus.com/inward/record.url?scp=39449134490&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=39449134490&partnerID=8YFLogxK
M3 - Article
AN - SCOPUS:39449134490
VL - 106
SP - 21565
EP - 21568
JO - Journal of Geophysical Research: Earth Surface
JF - Journal of Geophysical Research: Earth Surface
SN - 2169-897X
IS - A10
M1 - 2001JA000007
ER -