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Forbush decrease caused by interacting and non-interacting passing CME

Published online by Cambridge University Press:  27 November 2018

Mohamed Ismaiel
Mohamed Ismaiel*
Affiliation:
Space Weather Monitoring Center, Helwan University Ain Helwan 11798, Helwan, Egypt email: mohamed.r.emam@hotmail.com
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Abstract

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On 5-6 Aug. 2011 two short-time consecutive M-class solar flares led to profile of multiple Forbush Decreases showing the possible interaction of long-time passing of ICME.

Keywords

cosmic raysflarescoronal mass ejections (CMEs)Solar-stellar connection
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S340: Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles , February 2018 , pp. 151 - 152
Copyright
Copyright © International Astronomical Union 2018 

References

Belov, A. et al. Sci. Phys. 71–988/(2007).Google Scholar
Belov, A. et al. Sol Phys. 290–1429/(2015).Google Scholar
Enzl, J. et al. ISBN 978-80-7378-185-9/(2011).Google Scholar