• 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