Diffusive compression acceleration

Research output: Chapter in Book/Report/Conference proceedingChapter

5 Scopus citations

Abstract

We discuss the physics of diffusive compression acceleration of charged particles. This mechanism is similar to diffusive shock acceleration, which is well known, except that it applies to a gradual compression of the plasma, rather than a shock. It also applies to fluctuations in velocity, such as turbulence. We present the results from theoretical and numerical calculations for a variety of applications of this mechanism. These include: acceleration of particles by corotating solar-wind compressions, acceleration in a sinusoidally varying fluid flow, the formation of high-energy tails in pickup-ion distributions, and the acceleration of Galactic cosmic rays by turbulent flows in the interstellar medium. We also show that this mechanism naturally favors acceleration of particles with larger gyroradii. This may help explain recent observations of some solar-energetic particle observations showing abundance enhancements that increase with particle gyroradius.

Original languageEnglish (US)
Title of host publicationParticle Acceleration in Astrophysical Plasmas
Subtitle of host publicationGeospace and Beyond, 2005
EditorsJoseph Perez, Dennis Gallagher, John Quenby, Robert Preece, James Horwitz
PublisherBlackwell Publishing Ltd
Pages41-49
Number of pages9
ISBN (Electronic)9781118666104
ISBN (Print)9780875904214
DOIs
StatePublished - Jan 1 2005

Publication series

NameGeophysical Monograph Series
Volume156
ISSN (Print)0065-8448
ISSN (Electronic)2328-8779

ASJC Scopus subject areas

  • Geophysics

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