Cosmic-ray Diffusion
Cosmic-Ray Diffusion is a theoretical framework in astrophysics that describes the stochastic propagation of high-energy cosmic-ray particles through turbulent interstellar magnetic fields, distinguished from other transport mechanisms by its reliance on spatial and momentum-space diffusion coefficients derived from particle-scattering processes.
915
Publications
57.7K
Citations
1.5K
Authors
597
Institutions
Publications per year
2017–2026
169
Parents
915
Solar Modulation of Galactic Cosmic Rays
L. J. Gleeson, W. I. Axford · The Astrophysical Journal · 1968 · 1.2K citations
Natural Sciences, Astronomy, Physics +14
Propagation of Cosmic‐Ray Nucleons in the Galaxy
A. W. Strong, I. V. Moskalenko · The Astrophysical Journal · 1998 · 1.1K citations · Full text
Natural Sciences, Astronomy, Physics +16
1–5 of 915
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597

Centre National de la Recherche Scientifique
Paris, France
34 h-index
125 publications
8.3K citations

North-West University
Potchefstroom, South Africa
33 h-index
120 publications
5.6K citations
Goddard Space Flight Center
Greenbelt, United States
32 h-index
66 publications
4.7K citations
Ruhr University Bochum
Bochum, Germany
31 h-index
131 publications
5.5K citations
University of Maryland, College Park
College Park, United States
22 h-index
35 publications
2.4K citations

Chinese Academy of Sciences
Beijing, China
22 h-index
75 publications
2.8K citations
University of Chicago
Chicago, United States
21 h-index
37 publications
1.8K citations
University of Delaware
Newark, United States
21 h-index
48 publications
3.6K citations
1–8 of 597
ApJ · 221 publications · 20K citations
67
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70 publications · 4.6K citations
43
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JGR · 81 publications · 4.2K citations
38
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59 publications · 3.5K citations
36
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42 publications · 1.4K citations
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