Dynamics of isolated flare-related magnetic clouds in the quiet uniformly inhomogeneous inner heliosphere

Details Dynamics of isolated flare-related magnetic clouds in the quiet uniformly inhomogeneous inner heliosphere Dynamics of isolated flare-related magnetic clouds in the quiet uniformly inhomogeneous inner heliosphere

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..730i&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 30, Sept.-Oct. 1990, p. 730-735. In Russian.

Physics

2

Heliosphere, Magnetic Clouds, Magnetic Field Configurations, Solar Magnetic Field, Equations Of Motion, Solar Flares, Solar Wind

Scientific paper

Calculations of the transit velocities and times of the center of mass of a flare-related magnetic cloud from the sun to earth orbit are calculated for various flare positions with respect to the heliospheric current sheet and for various inclinations of this sheet to the plane of the solar equator. A powerful deceleration of the clouds is found as they propagate through a heliospheric streamer and the eastern periphery of the heliospheric current sheet.

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