Three-dimensional configuration and 'damping' effects of flare-generated coronal transients

Details Three-dimensional configuration and 'damping' effects of flare-generated coronal transients Three-dimensional configuration and 'damping' effects of flare-generated coronal transients

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..216i&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, Mar.-Apr. 1989, p. 216-221. In Russian.

Physics

Coronagraphs, Solar Flares, Stellar Mass Ejection, Shock Wave Propagation, Solar Corona, Transient Response

Scientific paper

The solution to the direct problem of the projection of coronal mass ejection (CME) of a given form on the celestial plane using white-light coronograph data is examined. The direct-problem solution is used to solve the inverse problem of searching for the three-dimensional configuration of the CME in the class of oblate spheropids. For Imax =2, it is shown that the transient has (in its front part) the form of an ellipsoid of revolution (with an axis ratio of about 1.25) oblate with respect to the plane of a great circle passing through the flare parallel to the magnetic axis of the nearest bipolar group.

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