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Coupling between the solar wind and the magnetosphere: CDAW 6

Journal Article · · J. Geophys. Res.; (United States)
Interplanetary conditions (VB/sub 3/, V/sup 2/B/sub 3/ and epsilon-c) are derived from ISEE 3 and IMP 8 field and plasma data for the two Coordinated Data Analysis Workshop (CDAW 6) intervals of study and are compared with various aspects of geomagnetic activity (AE, U/sub T/, derived Joule heating, electric potential, westward eastward and total electrojet currents). The March 22 (day 81), 1979, interval contains two distinct periods of geomagnetic activity, both highly correlated with interplanetary features. The start of the first active interval is caused by a southward turning of the interplanetary magnetic field (IMF) associated with the passage of a heliospheric current sheet. The start of the second interval is related to a second IMF southward turning. The geomagnetic activity intensifies when the second crossing of the current sheet, and a ram pressure increase of 4 to 6, impinges on the magnetosphere. Because the interplanetary parameters VB/sub 3/, V/sup 2/B/sub 3/ and epsilon-c decrease across the discontinuity, it is concluded that either additional energy is injected into the magnetosphere from the conversion of ram energy into magnetospheric substorm energy or some feature associated with current sheet crossing ''triggers'' the release of previously stored magnetosphere/magnetotail energy. It is not possible at this time to distinguish between these two possibilities. For day 81, VB/sub 3/, V/sup 2/4/sub 3/, and epsilon-c were highly correlated with AL, AE, westward and equivalent currents with coefficients ranging from approx.0.75 to 0.90.
Research Organization:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena
OSTI ID:
6025610
Journal Information:
J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 90:A2; ISSN JGREA
Country of Publication:
United States
Language:
English