Flare clouds as compact force-free toroidal configurations (According to VEGA 1 and 2 magnetic measurements)

Details Flare clouds as compact force-free toroidal configurations (According to VEGA 1 and 2 magnetic measurements) Flare clouds as compact force-free toroidal configurations (According to VEGA 1 and 2 magnetic measurements)

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kosis..26...57i&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 26, Jan.-Feb. 1988, p. 57-62. In Russian.

Computer Science

Interplanetary Flight, Interplanetary Magnetic Fields, Magnetic Field Configurations, Plasma Clouds, Solar Flares, Toroidal Plasmas, Plasma Interactions, Vega Project

Scientific paper

Experimental magnetic field profiles measured by Vega 1 and 2 as they passed through an interplanetary cloud on Feb. 16, 1986 are compared with approximate theoretical profiles derived from different assumptions on the structure of such clouds. Theory and experiment are found to agree best when the cloud is viewed as an oblate compact force-free toroid whose equatorial plane is approximately parallel to the plane of a great circle passing through the flare of Feb. 14, 1986 parallel to the magnetic axis closest to a bipolar-group flare.

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