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Manifestation of configurations of magnetic clouds of the solar wind in geomagnetic activity
Authors:N. A. Barkhatov  E. A. Kalinina  A. E. Levitin
Affiliation:(1) Nizhni Novgorod State Pedagogical University, Nizhni Novgorod, Russia;(2) Radiophysical Research Institute, Bol’shaya Pecherskaya ul. 25, GSP-51, Nizhni Novgorod, 603600, Russia;(3) Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Russian Academy of Sciences, Troitsk, Moscow oblast, 142190, Russia
Abstract:
On the basis of an analysis of the data of multi-satellite observations of magnetic clouds at the path Venus-Earth, the dependence of their geoeffectiveness on the orientation in the ecliptic plane and position relative to the Sun-Earth line is determined in the paper. The cloud parameters were determined on the basis of the model of a force-free cylindrical flux rope. The search for magnetic clouds in the flow of data from the monitoring space vehicle was performed using a special-purpose computer program.
Keywords:PACS 96.50.Uv
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