Computer Science – Sound
Scientific paper
Jan 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89..127p&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 89, Jan. 1, 1984, p. 127-135. Research supported by the Bundesministerium
Computer Science
Sound
37
Magnetic Field Configurations, Magnetopause, Satellite Sounding, Space Plasmas, Angles (Geometry), International Sun Earth Explorers, Magnetospheric Electron Density, Magnetospheric Proton Density
Scientific paper
Three passes of the ISEE 1 and 2 satellites through the dayside terrestrial magnetopause are discussed where the magnetopause is identified as a tangential discontinuity. This identification is based primarily on the failure of the plasma and magnetic field data to satisfy the conditions for a rotational discontinuity. In all these cases the interplanetary magnetic field was directed strongly southward and the angles between the fields on the two sides of the magnetopause ranged between 136 deg and 170 deg. As this is precisely the field geometry thought to be most conducive for reconnection, the magnetopause would be expected to be a rotational discontinuity. The simplest explanation of this result would appear to be that the magnetic field orientation is not the only factor controlling the onset of reconnection. However, as the identification of the discontinuity applies only locally, it cannot be excluded that for the magnetic field conditions investigated here, different portions of the magnetopause can be described as tangential and rotational discontinuities simultaneously.
Bame J. Jr. S.
Berchem Jean
Papamastorakis Ioannis
Paschmann Goetz
Sckopke Norbert
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