Abundances and spectra of superathermal H(+), He(++) and heavy ions in a fast moving plasma structure (plasmoid) in the distant geotail

Details Abundances and spectra of superathermal H(+), He(++) and heavy ions in a fast moving plasma structure (plasmoid) in the distant geotail Abundances and spectra of superathermal H(+), He(++) and heavy ions in a fast moving plasma structure (plasmoid) in the distant geotail

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984georl..11..603g&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 11, June 1984, p. 603-606. Sponsorship: Bundesministerium für Forschung und

Physics

37

Energetic Particles, Energy Spectra, Geomagnetic Tail, Heavy Ions, Helium Ions, Hydrogen Ions, Plasma Spectra, Space Plasmas, Abundance, Convective Flow, Distribution Functions, International Sun Earth Explorer 3, Positive Ions, Solar Wind

Scientific paper

An ISEE-3 Geotail Mission sensor has furnished data on a 16-min particle intensity increase in the distant magnetotail from which rest frame distribution functions have been deduced for 3-150 keV/amu H(+), He(++), and ions with a charge state greater than 3. The event was characterized by isotropic electron distributions and is identified as a tailward-moving plasmoid. These suprathermal ions are convected nearly tailward at an average speed of 1000 + or - 50 km/sec and have an energy density of 150 eV/cu cm. A crosstail expansion speed of about 80 km/sec is indicated.

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