Computer Science
Scientific paper
Sep 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20..645l&link_type=abstract
Advances in Space Research, vol. 20, n, p. 645
Computer Science
5
Solar Wind, Shock Wave Propagation, Energetic Particles, Plasma Diagnostics, Satellite Imagery, Bow Waves, Satellite-Borne Instruments
Scientific paper
The 3D Plasma and Energetic Particles Experiment on the WIND spacecraft provides high sensitivity, wide dynamic range, good energy and angular resolution, full 3-D coverage, and high time resolution over the energy range from a few eV to greater than 300 keV for electrons and greater than about 6 MeV for ions. Results are reported for electrons from the first year of operation. These include: the detection of a quiet-time 'super-halo' component of interplanetary electrons from about 1 to 100 keV; the discovery that the spectrum of impulsive solar electron events extends down to as low as about 0.5 keV energy; the remote probing of the Earth's bow shock; and detailed studies of the electron beam/plasma wave interaction responsible for solar type II radio bursts.
Anderson Katharine A.
Ashford S.
Bosqued Jean Michel
Carlson Carl W.
D'Uston Claude
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