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Outer Plasmaspheric Plasma Properties: What We Know from Satellite Data

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Abstract

Our understanding of the composition, density, and temperature structure of the outer plasmasphere has undergone several major revisions since the discovery of the plasmasphere over 35 years ago. Each new era of understanding was brought about by the launching of satellites carrying suites of plasma diagnostic experiments each more sophisticated than its predecessor. Instead of each new generation of missions providing incremental advancement in our knowledge of the plasmasphere's plasma properties, they most often than not, initiated a complete re-thinking of our understanding. There are still a number of observational "puzzles" and large gaps in our knowledge of how plasmaspheric structure and plasma properties change with geomagnetic storm and substorm activity. As we develop new missions to attempt to globally image the outer plasmasphere in order to put simultaneous multi-spacecraft observations into context, we undoubtedly will uncover new tantalizing observations that will cause us to re-think our mental picture of the plasmasphere. What we have learned from satellite data about the chemical composition, density, temperature and pitch-angle distribution properties and their variability is outlined in this review paper.

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  1. Department of Physics and Space Sciences, Florida Institute of Technology, Melbourne, Florida, USA

    Mark B. Moldwin

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Moldwin, M.B. Outer Plasmaspheric Plasma Properties: What We Know from Satellite Data. Space Science Reviews 80, 181–198 (1997). https://doi.org/10.1023/A:1004921903897

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