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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
Case study of Forbush decreases: Energy dependence of the recovery
Advances in Space Research, 2007Ilya G Usoskin
exaly
Power Law Distribution of Forbush Decrease Magnitude
Research Notes of the AAS, 2018A. A. Melkumyan +6 more
openaire +1 more source
Cloudiness decreases associated with Forbush-decreases of galactic cosmic rays
Journal of Atmospheric and Solar-Terrestrial Physics, 1995Svetlana V Veretenenko
exaly
Galactic cosmic ray spectral index: the case of Forbush decreases of March 2012
Astrophysics and Space Science, 2017Helen Mavromichalaki, Christina Plainaki
exaly
Precursor Effects in Different Cases of Forbush Decreases
Solar Physics, 2011Helen Mavromichalaki +2 more
exaly
Two intense Forbush decreases of solar activity cycle 22
Advances in Space Research, 2009Hs Ahluwalia
exaly
Forbush decreases: Origin and development in the interplanetary space
Il Nuovo Cimento Della Società Italiana Di Fisica C, 1979exaly

