Publication Date:
2011-08-24
Description:
The interaction of the thermosphere and ionosphere is largely governed by collisions between ions and neutral particles. On Venus and the Earth, O(+) is a dominant ion, and atomic O dominates throughout much of the thermosphere; therefore an accurate O(+)-O cross section is an important prerequisite for understanding the dynamics of planetary upper atmospheres. The cross section and momentum transfer collision frequency are calculated with a quantum mechanical code which includes resonance charge exchange, polarization, and charge-quadrupole effects. Our results agree well with earlier calculations of Stubbe (1968) and Stallcop et al. (1991).
Keywords:
LUNAR AND PLANETARY EXPLORATION
Type:
Geophysical Research Letters (ISSN 0094-8276); 20; 13; p. 1343-1346.
Format:
text