Computer Science – Numerical Analysis
Scientific paper
Feb 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988angeo...6..113l&link_type=abstract
Annales Geophysicae (ISSN 0980-8752), vol. 6, Feb. 1988, p. 113-128.
Computer Science
Numerical Analysis
43
Bow Waves, Electromagnetic Radiation, Geomagnetism, Plasma Frequencies, Solar Wind, Space Plasmas, Hot Electrons, International Sun Earth Explorers, Numerical Analysis, Radio Waves, Wave Scattering
Scientific paper
Oservations of radiation produced in the vicinity of the earth's bow shock at twice the solar wind electron plasma frequency have been obtained by ISEE-1 at about 20 earth radii and by ISEE-2 at about 200 earth radii from the earth. The source of this electromagnetic radiation is shown to be near the upstream boundary of the foreshock, the surface where the magnetic field lines are tangent to the bow shock. For a source of thickness of 1 earth radius, the emissivity is found to be 0.5-20 x 10 to the -22nd W/cu m per sr. Observations are compared with the predictions of current source models.
Harvey Chris
Hoang Sang
Lacombe Catherine
Mangeney Andre
Steinberg Jean-Louis
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