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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 in
openaire   +1 more source

Case study of Forbush decreases: Energy dependence of the recovery

Advances in Space Research, 2007
Ilya G Usoskin
exaly  

Power Law Distribution of Forbush Decrease Magnitude

Research Notes of the AAS, 2018
A. A. Melkumyan   +6 more
openaire   +1 more source

Geomagnetic storms, Forbush decreases of cosmic rays and total ozone at northern higher middle latitudes

Journal of Atmospheric and Solar-Terrestrial Physics, 2005
Jan Lastovicka
exaly  

Cloudiness decreases associated with Forbush-decreases of galactic cosmic rays

Journal of Atmospheric and Solar-Terrestrial Physics, 1995
Svetlana V Veretenenko
exaly  

Galactic cosmic ray spectral index: the case of Forbush decreases of March 2012

Astrophysics and Space Science, 2017
Helen Mavromichalaki, Christina Plainaki
exaly  

Precursor Effects in Different Cases of Forbush Decreases

Solar Physics, 2011
Helen Mavromichalaki   +2 more
exaly  

Two intense Forbush decreases of solar activity cycle 22

Advances in Space Research, 2009
Hs Ahluwalia
exaly  

Forbush decreases: Origin and development in the interplanetary space

Il Nuovo Cimento Della Società Italiana Di Fisica C, 1979
exaly  

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