Bow Shock Physics
Bow Shock Physics is a theoretical framework that characterizes the nonlinear interaction and energy dissipation processes of supersonic magnetized plasmas at the boundary preceding a planetary magnetosphere, distinguished by its focus on collisionless shock formation, particle acceleration, and field compression mechanisms in space environments.
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2017–2026
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A Textbook Example of a Bow Shock in the Merging Galaxy Cluster 1E 0657-56
Maxim Markevitch, Anthony H. Gonzalez, L. P. David et al. · The Astrophysical Journal · 2002 · 624 citations · Full text
Natural Sciences, Astronomy, Physics +13
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Goddard Space Flight Center
Greenbelt, United States
77 h-index
580 publications
42.8K citations
University of California, Los Angeles
Los Angeles, United States
67 h-index
317 publications
21.3K citations
Planetary Science Institute
Tucson, United States
52 h-index
241 publications
14.3K citations
University of California, Berkeley
Berkeley, United States
52 h-index
395 publications
22.7K citations

Imperial College London
London, United Kingdom
47 h-index
285 publications
12.9K citations
University of Iowa
Iowa City, United States
47 h-index
184 publications
10.6K citations
Los Alamos National Laboratory
Los Alamos, United States
46 h-index
170 publications
14.8K citations

Centre National de la Recherche Scientifique
Paris, France
44 h-index
429 publications
20.9K citations
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JGR · 647 publications · 42.2K citations
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ApJ · 252 publications · 15.8K citations
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245 publications · 11.7K citations
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180 publications · 6.9K citations
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111 publications · 5.8K citations
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