Deceleration and acceleration of cosmic rays in the solar wind

Research output: Contribution to journalArticle

20 Citations (Scopus)

Abstract

Recent observations of the deceleration of low-energy solar cosmic rays in the solar wind are discussed in the context of cosmic-ray transport theory. It is concluded that the rate of deceleration is much slower than would be produced by adiabatic energy change due to the observed expansion of the plasma, so that a competing acceleration process must be operative. Second-order Fermi acceleration by hydromagnetic waves, acting together with adiabatic energy change, is shown to provide a natural interpretation of the observations.

Original languageEnglish (US)
Pages (from-to)666-669
Number of pages4
JournalPhysical Review Letters
Volume26
Issue number11
DOIs
StatePublished - 1971
Externally publishedYes

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deceleration
solar wind
cosmic rays
solar cosmic rays
transport theory
magnetohydrodynamic waves
energy
expansion

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Deceleration and acceleration of cosmic rays in the solar wind. / Jokipii, J. Randy.

In: Physical Review Letters, Vol. 26, No. 11, 1971, p. 666-669.

Research output: Contribution to journalArticle

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