Plasma and energetic particles in the magnetotail at 60 earth radii

Details Plasma and energetic particles in the magnetotail at 60 earth radii Plasma and energetic particles in the magnetotail at 60 earth radii

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974jgr....79.4779c&link_type=abstract

Journal of Geophysical Research, vol. 79, Nov. 1, 1974, p. 4779-4785. DOD-AEC-sponsored research;

Physics

4

Apollo Flights, Energy Spectra, Geomagnetic Tail, High Energy Electrons, Plasma Diagnostics, Earth Magnetosphere, Electron Energy, Electrostatic Probes, Lunar Orbits, Magnetosheath, Maxwell-Boltzmann Density Function, Polar Substorms, Satellite Observation, Solar Wind

Scientific paper

Particle measurements made by the lunar-orbiting Apollo subsatellites have shown that electron energy spectra in the range 0.55-320 keV in the high-latitude magnetotail often fit a power law with an exponent of -3 and a flux at .5 keV of 200,000 to 700,000 el/sq cm s sr keV. In the magnetosheath, electron energy spectra are similar to the high-latitude magnetotail spectra. In the plasma sheet, electron energy spectra often fit the high-energy tail of a Maxwellian distribution with Eo of about 200-500 eV. During times of substorms a number of cases where the plasma sheet appears to thin at onset have been observed. In addition, cases of plasma sheet expansion at onset have also been observed.

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