A simulation study of distortion of the heliospheric sheet caused by solar activity

Details A simulation study of distortion of the heliospheric sheet caused by solar activity A simulation study of distortion of the heliospheric sheet caused by solar activity

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985p%26ss...33..925f&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 33, Aug. 1985, p. 925-931.

Physics

6

Current Sheets, Heliosphere, Interplanetary Magnetic Fields, Magnetic Field Configurations, Solar Activity Effects, Magnetic Storms, Solar Flares, Solar Wind Velocity

Scientific paper

During major geomagnetic storms, the interplanetary magnetic field angle, phi, changes often abruptly, either from 135 to 315 or 315 to 135 deg, suggesting that the heliospheric current sheet is pushed upward or downward by disturbed solar wind. The distortion of the heliospheric current sheet by three successive solar flares is simulated to show that such a flapping motion can occur.

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