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Modeling of Forbush decreases in cosmic rays
An explosion at the Sun that releases a large amount of mass with high velocity, known as a coronal mass ejection (CME), causes a discontinuity in the solar wind known as a shock. The shock and associated energetic cosmic rays could cause various problems for human activities known as "space weather effects." This work studies the particle transport inopenaire +1 more source
Gnevyshev gap, Forbush decreases, ICMEs and solar wind electric field: relationships
Advances in Space Research, 2005H S Ahluwalia
exaly
The catalog of Forbush decreases across heliosphere
We aim to compile an extensive catalog of Forbush decreases (FDs) caused by interplanetary coronal mass ejections (ICMEs), using ground-based as well as instruments from various spacecraft across heliosphere. Forbush decreases are short term depressions of galactic cosmic ray flux and one of the common signatures of interplanetary coronal mass ...Dumbović, Mateja +1 more
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Forbush decreases of cosmic rays: Energy dependence of the recovery phase
Journal of Geophysical Research, 2008I G Usoskin, I Braun, J R Hörandel
exaly
Case study of Forbush decreases: Energy dependence of the recovery
Advances in Space Research, 2007I G Usoskin, T Raiha, J Sarkamo
exaly