Physics
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..120..407i&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 120, no. 2, 1989, p. 407-419.
Physics
37
Clouds, Interplanetary Magnetic Fields, Magnetic Field Configurations, Solar Flares, Force-Free Magnetic Fields, Shock Waves, Toroids, Vega Project
Scientific paper
Simple models of the geometry, structure, and dynamics of magnetic clouds are developed using magnetic measurements made by Vega 1 and Vega 2 during the solar-interplanetary events in January and February of 1986. The results confirm the idea of a flare-generated magnetic cloud as a compact oblate force-free toroid, the equatorial plane of which is parallel to the plane of the great circle passing through a flare parallel to the magnetic axis of the bipolar group of solar spots which is closest to the flare. The geometric and kinematic characteristics of the clouds can in principle agree with the theory of the movement of these clouds from the sun under the effect of magnetic buoyancy, gravitation, and hydrodynamic deceleration.
Eroshenko E. G.
Harshiladze A. F.
Ivanov K. G.
Stiazhkin V. A.
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