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Cross Sections and Reaction Rates for Comparative Planetary Aeronomy

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Abstract

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.

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Authors and Affiliations

  1. Molecular Physics Laboratory, SRI International, Menlo Park, CA, 94025, USA

    David L. Huestis

  2. Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI, 48109, USA

    Stephen W. Bougher

  3. Department of Physics, Wright State University, Dayton, OH, 45435, USA

    Jane L. Fox

  4. Space and Atmospheric Physics, Imperial College London, London, SW7 2AZ, UK

    Marina Galand & Juliet C. Pickering

  5. Engineering Physics and Materials Science, University of Virginia, Charlottesville, VA, 22904, USA

    Robert E. Johnson

  6. Planetary Science, Lunar and Planetary Institute, Houston, TX, 77058, USA

    Julianne I. Moses

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Prepared for publication in Space Science Reviews (Springer) and in the International Space Science Institute (ISSI Bern) book series, Volume 29.

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Huestis, D.L., Bougher, S.W., Fox, J.L. et al. Cross Sections and Reaction Rates for Comparative Planetary Aeronomy. Space Sci Rev 139, 63–105 (2008). https://doi.org/10.1007/s11214-008-9383-7

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