Cross Sections and Reaction Rates for Comparative Planetary Aeronomy

被引：71
作者：
Huestis, David L. [1 ]
Bougher, Stephen W. [2 ]
Fox, Jane L. [3 ]
Galand, Marina [4 ]
Johnson, Robert E. [5 ]
Moses, Julianne I. [6 ]
Pickering, Juliet C. [4 ]
机构：
[1] SRI Int, Mol Phys Lab, Menlo Pk, CA 94025 USA
[2] Univ Michigan, Ann Arbor, MI 48109 USA
[3] Wright State Univ, Dept Phys, Dayton, OH 45435 USA
[4] Univ London Imperial Coll Sci Technol & Med, London SW7 2AZ, England
[5] Univ Virginia, Charlottesville, VA 22904 USA
[6] Lunar & Planetary Inst, Houston, TX 77058 USA
来源：
SPACE SCIENCE REVIEWS | 2008年 / 139卷 / 1-4期
关键词：
Collisions; Photoabsorption; Chemical reactions; Critical evaluation; Laboratory measurement; First-principles theory; Needs in atmospheric models;
D O I：
10.1007/s11214-008-9383-7
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this chapter we describe the current knowledge of a selection of collision processes and chemical reactions of importance to planetary aeronomy. Emphasis is placed on critical evaluation of what we know and what we wish we knew about fundamental processes required for interpretation, explanation, and modeling of atmospheric observations.
引用
收藏
页码：63 / 105
页数：43
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