Computer Science
Scientific paper
Sep 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..587v&link_type=abstract
In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2
Computer Science
Magnetic Clouds, Interplanetary Magnetic Field, Field Draping
Scientific paper
Magnetic clouds are known as a possible source of strong geomagnetic storms due to a large southward Bz component located in their interior. Magnetic clouds as magnetically isolated bodies also disturb the ambient magnetic field around them during their propagation. This draped field may contain significantly large southward Bz component and thus it may also cause a geomagnetic storm. Therefore the knowledge on the draped field is important for space weather predictions. Theoretical external magnetic field profiles (assumed to be potential) are compared with real measurements of magnetic fields near magnetic clouds for several events. From 15 analyzed cases about one half was found to be consistent with the model, one fifth not, and remaining cases were not able to be evaluated due to large fluctuations.
Romashets E. P.
Vandas Marek
Watari Shinichi
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