The Identification of a Planar Magnetic Structure within the ICME Shock Sheath and Its influence on Galactic Cosmic-Ray Flux
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/866/i=2/a=118/pdf
Reference74 articles.
1. High-rigidity Forbush decreases: due to CMEs or shocks?
2. Solar Energetic Particle Transport Near a Heliospheric Current Sheet
3. What determines the magnitude of forbush decreases?
4. Forbush effects and their connection with solar, interplanetary and geomagnetic phenomena
5. RELATIVE CONTRIBUTION OF THE MAGNETIC FIELD BARRIER AND SOLAR WIND SPEED IN ICME-ASSOCIATED FORBUSH DECREASES
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3. In Situ Observation of Alfvén Waves in an ICME Shock-Sheath Indicating the Existence of Alfvénic Turbulence;Solar Physics;2024-03
4. The role of extreme geomagnetic storms in the Forbush decrease profile observed by neutron monitors;Journal of Atmospheric and Solar-Terrestrial Physics;2023-11
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