Far Ultraviolet Remote Sensing of Venus and Mars

  1. Janet G. Luhmann,
  2. Mariella Tatrallyay and
  3. Robert O. Pepin
  1. Larry J. Paxton1 and
  2. Donald E. Anderson2

Published Online: 18 MAR 2013

DOI: 10.1029/GM066p0113

Venus and Mars: Atntospheres, Ionospheres, and Solar Wind Interactions

Venus and Mars: Atntospheres, Ionospheres, and Solar Wind Interactions

How to Cite

Paxton, L. J. and Anderson, D. E. (1992) Far Ultraviolet Remote Sensing of Venus and Mars, in Venus and Mars: Atntospheres, Ionospheres, and Solar Wind Interactions (eds J. G. Luhmann, M. Tatrallyay and R. O. Pepin), American Geophysical Union, Washington, D. C.. doi: 10.1029/GM066p0113

Author Information

  1. 1

    Johns Hopkins University, Applied Physics Laboratory

  2. 2

    Computational Physics, Inc.

Publication History

  1. Published Online: 18 MAR 2013
  2. Published Print: 1 JAN 1992

ISBN Information

Print ISBN: 9780875900322

Online ISBN: 9781118663844

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Keywords:

  • Venus (Planet)—Atmosphere—Congresses;
  • Mars (Planet)—Atmosphere—Congresses;
  • Solar wind—Congresses

Summary

This chapter contains sections titled:

  • Introduction

  • UV Remote Sensing

  • Model Inputs

  • Review of UV Observations

  • HI 1216

  • OI 1304

  • CO Fourth Positive Group Bands

  • CI 1657 and 1561

  • EUV Emissions

  • Future Missions

  • Summary and Conclusions