Cosmic ray modulation by solar wind disturbances
Mateja Dumbović, B. Vršnak, Jaša Čalogović, M. Karlica
Abstract
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Mateja Dumbović, B. Vršnak, Jaša Čalogović, M. Karlica
Abstract
Open-access reader
Aims. We perform a systematic statistical study of the relationship between characteristics of solar wind disturbances, caused by interplanetary coronal mass ejections and corotating interaction regions, and properties of Forbush decreases (FDs). Since the mechanism of FDs is still being researched, this analysis should provide a firm empirical basis for physical interpretations of the FD phenomenon.
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Aims. We perform a systematic statistical study of the relationship between characteristics of solar wind disturbances, caused by interplanetary coronal mass ejections and corotating interaction regions, and properties of Forbush decreases (FDs). Since the mechanism of FDs is still being researched, this analysis should provide a firm empirical basis for physical interpretations of the FD phenomenon.
Key concepts: Physics, Coronal mass ejection, Solar wind, Interplanetary spaceflight, Forbush decrease, Astrophysics, Interplanetary medium, Cosmic ray