Hostname: page-component-848d4c4894-xfwgj Total loading time: 0 Render date: 2024-07-01T10:54:07.788Z Has data issue: false hasContentIssue false
  • English
  • Français

Streaming of Solar Cosmic Rays

Published online by Cambridge University Press:  25 April 2016

K. G. McCracken  and
I. D. Palmer
K. G. McCracken
Affiliation:
Department of Physics, University of Adelaide
I. D. Palmer
Affiliation:
Department of Physics, University of Adelaide
Get access Rights & Permissions [Opens in a new window]

Extract

A comprehensive study of the anisotropy (i.e. streaming) of solar cosmic rays at energies ~10 MeV revealed two distinct types (McCracken). The first occurs during onset phase of the event, is large (> 20%), and is really the flow of cosmic rays along lines of force driven by a density gradient. The second describes the decay of the event, is small (10%), and indicates a flow radially away from the Sun.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 6 , September 1969 , pp. 276 - 278
Copyright
Copyright © Astronomical Society of Australia 1969

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 McCracken, K. G. et al., J.G.R., 72, 4293 (1967).Google Scholar
2 Ahluwalia, A. S. and Dessler, A. J., Planet. Sp. Sc, 9, 195 (1962).Google Scholar
3 Gleeson, L. J., Planet. Sp. Sc., 17, 31 (1969).Google Scholar