Interplanetary Transient Plasma Signatures and Associated Cosmic Ray Intensity Variation

Details Interplanetary Transient Plasma Signatures and Associated Cosmic Ray Intensity Variation Interplanetary Transient Plasma Signatures and Associated Cosmic Ray Intensity Variation

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3735k&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

Two types of interplanetary (IP) transient disturbances, namely magnetic cloud events (MCEs) and bidirectional events (BDEs) are analyzed to study the shortterm changes in the solar wind (SW) plasma components as well as in cosmic ray intensity. Thses disturbances are divided in to two categories: coronal holes (CH) associated events and without CH associated events to analyze their influences explicitly. Study reveal distinctly different effects on SW plasma velocity and cosmic ray intensity. The BDEs associated with CH are found significantly responsible for enhanced plasma velocity. Both disturbances (MCEs and BDEs) produce decrease in cosmic ray intensity, but lesser decrease and fast recoveries are evident in case of events associated with CH.

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