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Title: Origins of magnetospheric plasma

Conference · · Reviews of Geophysics and Space Physics; (United States)
OSTI ID:5027282
 [1]
  1. USAF, Geophysics Laboratory, Hanscom AFB, MA (United States)

A review is given of recent (1987-1990) progress in understanding of the origins of plasmas in the earth's magnetosphere. In counterpoint to the early supposition that geomagnetic phenomena are produced by energetic plasmas of solar origin, 1987 saw the publication of a provocative argument that accelerated ionospheric plasma could supply all magnetospheric auroral and ring current particles. Significant new developments of existing data sets, as well as the establishment of entirely new data sets, have improved the ability to identify plasma source regions and to track plasma through the magnetospheric system of boundary layers and reservoirs. These developments suggest that the boundary between ionospheric and solar plasmas, once taken to lie at the plasmapause, actually lies much nearer to the magnetopause. Defining this boundary as the surface where solar wind and ionosphere contribute equally to the plasma, it is referred to herein as the 'geopause'. It is now well established that the infusion of ionospheric O(+) plays a major role in the storm-time distention of the magnetotail and inflation of the inner magnetosphere. After more than two decades of observation and debate, the question remains whether magnetosheric are protons of solar or terrestrial origin. 161 refs.

OSTI ID:
5027282
Report Number(s):
CONF-910878-; CODEN: RGPSB
Journal Information:
Reviews of Geophysics and Space Physics; (United States), Vol. 29; Conference: 20. general assembly of the International Union of Geodesy and Geophysics (IUGG), Vienna (Austria), 11-24 Aug 1991; Related Information: Shea, M. A; ISSN 0034-6853
Country of Publication:
United States
Language:
English