A kinky heliospheric current sheet - Cause of CDAW-6 substorms

Details A kinky heliospheric current sheet - Cause of CDAW-6 substorms A kinky heliospheric current sheet - Cause of CDAW-6 substorms

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984georl..11..339t&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 11, April 1984, p. 339-342.

Physics

24

Current Sheets, Interplanetary Magnetic Fields, Interplanetary Medium, Magnetic Storms, Magnetospheric Instability, Solar Terrestrial Interactions, Heliosphere, Magnetic Clouds, Shock Waves, Solar Wind

Scientific paper

Two magnetospheric substorms and the intensification of the second are caused by interplanetary magnetic field and ram pressure changes associated with a kinky heliospheric current sheet (KHCS). The responsible interplanetary features occur in a highly compressed region between a solar flare-associated shock wave and the cold driver gas. The possibility that the interplanetary structure is a 'magnetic cloud' is ruled out.

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