Low-energy cosmic-ray modulation related to observed interplanetary magnetic field irregularities

G. Gloeckler, J. Randy Jokipii

Research output: Contribution to journalArticle

15 Citations (Scopus)

Abstract

The diffusion coefficient describing the motion of cosmic-ray particles in the interplanetary magnetic field is determined from the power spectrum of magnetic irregularities observed on space probes, and is found to be proportional to R (R=particle magnetic rigidity, =particle velocity). Near minimum solar activity, only this dependence of the diffusion coefficient on R and can account for the observed long-term intensity variations of cosmic-ray protons and helium nuclei down to 10 MeV per nucleon in energy. Thus, the motion of cosmic rays in interplanetary space may be quantitatively related to the observed magnetic field.

Original languageEnglish (US)
Pages (from-to)203-207
Number of pages5
JournalPhysical Review Letters
Volume17
Issue number4
DOIs
StatePublished - 1966
Externally publishedYes

Fingerprint

interplanetary magnetic fields
irregularities
cosmic rays
modulation
diffusion coefficient
magnetic rigidity
space probes
interplanetary space
solar activity
energy
power spectra
helium
nuclei
protons
magnetic fields

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Low-energy cosmic-ray modulation related to observed interplanetary magnetic field irregularities. / Gloeckler, G.; Jokipii, J. Randy.

In: Physical Review Letters, Vol. 17, No. 4, 1966, p. 203-207.

Research output: Contribution to journalArticle

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