DocumentCode
1436800
Title
Core plasmas in space weather regions
Author
Horwitz, James L. ; Moore, Thomas E.
Author_Institution
Dept. of Phys., Alabama Univ., Huntsville, AL, USA
Volume
28
Issue
6
fYear
2000
fDate
12/1/2000 12:00:00 AM
Firstpage
1840
Lastpage
1853
Abstract
In recent years, there has been strong interest in “space weather,” owing to increasing recognition of the myriad effects that such phenomena may have on space and even ground systems of considerable importance to man. The authors describe the presence of “core” plasmas in the ionosphere and magnetosphere, which may influence various space weather phenomena. Core plasmas are defined as plasmas with energies from zero to 50 eV (Horowitz, Rev. Geophys., 1987) and originating in the terrestrial ionosphere. They first describe the ionosphere as the basic core plasma region for the overall magnetosphere-ionosphere system. They then describe the principal inner/middle magnetospheric regions-the plasmasphere, ring current, and plasma sheet regions-and how core plasmas from the ionosphere, either with little or with substantial energization, become major components of these magnetospheric regions, which are prime “space weather” regions
Keywords
ionosphere; magnetosphere; solar wind; core plasma; ionosphere; low energy plasma; magnetosphere; magnetosphere-ionosphere system; plasma; plasma sheet; plasmasphere; ring current; solar wind interaction; solar wind magnetosphere interaction; space weather; Extraterrestrial measurements; Extraterrestrial phenomena; Ionosphere; Magnetic cores; Magnetosphere; Physics; Plasma measurements; Plasma properties; Storms; Weather forecasting;
fLanguage
English
Journal_Title
Plasma Science, IEEE Transactions on
Publisher
ieee
ISSN
0093-3813
Type
jour
DOI
10.1109/27.902213
Filename
902213
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