Volume 301 -
35th International Cosmic Ray Conference (ICRC2017) -
Session Solar & Heliospheric. SH-Transient solar phenomena (SEP, GLE, Forbush decreases)
Theory of Forbush Decrease in a Magnetic Cloud
Full text:
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Pre-published on:
August 16, 2017
Published on:
August 03, 2018
Abstract
A model of Forbush-decrease in a magnetic cloud is presented. We calculate moments of the particle distribution function depending on time. The calculated results of cosmic ray intensity generally agree with the observed ones in events registered by ground based detectors. It is found that the magnetic flux rope is of great importance in dynamics of Forbush decrease.
DOI: https://doi.org/10.22323/1.301.0122
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.