Suprathermal O(+) and H(+) ion behavior during the March 22, 1979 (CDAW 6), substorms

Details Suprathermal O(+) and H(+) ion behavior during the March 22, 1979 (CDAW 6), substorms Suprathermal O(+) and H(+) ion behavior during the March 22, 1979 (CDAW 6), substorms

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jgr....90.1263i&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 90, Feb. 1, 1985, p. 1263-1272. Sponsorship: Bundesministerium für Forsch

Physics

22

Hydrogen Ions, Magnetic Storms, Magnetospheric Instability, Magnetospheric Ion Density, Oxygen Ions, Plasma Diagnostics, Energetic Particles, Geomagnetic Tail, Helium Ions, Plasma Layers, Positive Ions, Space Plasmas, Time Response

Scientific paper

The present investigation has the objective to report on the behavior of energetic (approximately 130 keV) O(+) ions in the earth's plasma sheet, taking into account observations by the ISEE 1 spacecraft during a magnetically active time interval encompassing two major substorms on March 22, 1979. Attention is also given to suprathermal H(+) and He(++) ions. ISEE 1 plasma sheet observations of the proton and alpha particle phase space densities as a function of energy per charge during the time interval 0933-1000 UT on March 22, 1979 are considered along with the proton phase space density versus energy in the energy interval approximately 10 to 70 keV for the selected time periods 0933-1000 UT (presubstorm) and 1230-1243 UT (recovery phase) during the 1055 substorm on March 22, 1979. A table listing the proton energy density for presubstorm and recovery periods is also provided.

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