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The acceleration of cosmic rays in shock fronts – I

A. R. Bell
- 01 Feb 1978 - 
- Vol. 182, Iss: 2, pp 147-156
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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1978-02-01 and is currently open access. It has received 2613 citations till now. The article focuses on the topics: Shock waves in astrophysics & Fermi acceleration.

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Proton-Helium Spectral Anomaly as a Signature of Cosmic Ray Accelerator

TL;DR: By fitting the p/He ratio to the PAMELA data, the diffusive shock acceleration case for resolving the century-old mystery of CR origin is bolstered, and it is demonstrated that the spectral difference is a unique signature of the acceleration mechanism.
Journal ArticleDOI

Non-linear diffusion of cosmic rays

TL;DR: In this paper, a self-similar solution of the equation of non-linear diffusion for particles ejected from a supernova source is presented, and the results may change the physical picture of cosmic ray propagation in the Galaxy.
Journal ArticleDOI

Compression Acceleration in Astrophysical Plasmas and the Production of f(v) v ?5 Spectra in the Heliosphere

TL;DR: In this paper, a new derivation of the acceleration of fast charged particles by random compressions and expansions based on a quasilinear approximation applied to the Parker transport equation is presented.
Journal ArticleDOI

Open Questions in Cosmic-Ray Research at Ultrahigh Energies

TL;DR: In this paper, the authors review open questions and prospects for progress in ultra-high-energy cosmic ray (UHECR) research, based on a series of discussions that took place during the ''The High-Energy Universe: Gamma-Ray, Neutrino and Cosmic-ray Astronomy' MIAPP workshop in 2018.
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