Physics
Scientific paper
Mar 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985georl..12..129g&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 12, March 1985, p. 129-132.
Physics
18
Angles (Geometry), International Sun Earth Explorers, Interplanetary Magnetic Fields, Shock Fronts, Solar Terrestrial Interactions, Convection, Extremely Low Frequencies, Ions, Magnetic Flux, Solar Wind
Scientific paper
Saturated ULF waves in the foreshock, with amplitudes comparable to the magnitude of the average field, are convected by the solar wind to the quasi-parallel shock where the average field-normal angle is less than, or about, 45 deg. Several examples from ISEE 1 and 2 magnetometer data show waves that defined local, instantaneous field-normal angles very different periodically from the average. Local geometric conditions at the nominally quasi-parallel shock varied from nearly parallel to nearly perpendicular, at the periods of typical upstream waves. Clear magnetic shock transitions occurred under temporarily quasi-perpendicular geometry.
Greenstadt Eugene W.
Mellott Mary M.
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