The Technique of Forbush Decrease Registration in Tomography Mode

Details The Technique of Forbush Decrease Registration in Tomography Mode The Technique of Forbush Decrease Registration in Tomography Mode

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3627b&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

A new method of studies of dynamic processes in heliosphere by means of muon ho doscope with a high angular resolution is considered. Coronal mass ejections produce dynamic inhomogeneities in interplanetary magnetic field (IMF). Ho doscope continuously registers flux of muons from 65025 spatial directions. The simultaneous observation of cosmic ray flux from various directions as a sequence of two-dimensional "muon-graphs" with high angular resolution allows to study dynamic picture of IMF.

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