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Cited by 501

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Cosmic Ray Streaming--I EFFECT OF ALFVEN WAVES ON PARTICLES

Open access
Skilling, J.·1975·Monthly Notices of the Royal Astronomical Society

Abstract

The motion of cosmic rays through a moving magnetized medium supporting a spectrum of hydromagnetic waves is re-examined. In different approximations, Fermi acceleration, convective motion through space, diffusive motion, and free streaming are recovered. It is shown that Fermi acceleration can greatly modify the adiabatic energy losses which have conventionally been thought to accompany convective motion of cosmic rays. This may have implications for ‘ self-confinement ’ theories of cosmic ray propagation.

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Crossref · 10.1093/mnras/172.3.557

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Metadata

Authors
Skilling, J.
Venue
Monthly Notices of the Royal Astronomical Society
Published
1975-09-01
Volume
172
Issue
3
Pages
557-566
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W1983072771
Cited by
501
References
0
FWCI
0.68
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Cosmic Ray Streaming--I EFFECT OF ALFVEN WAVES ON PARTICLES. https://app.cochat.ai/papers/10.1093/mnras/172.3.557
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Skilling, J. (1975). Cosmic Ray Streaming--I EFFECT OF ALFVEN WAVES ON PARTICLES. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/172.3.557

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.