Cosmic-ray solar-flare increase of 28 January 1967
- 15 May 1968
- journal article
- Published by Canadian Science Publishing in Canadian Journal of Physics
- Vol. 46 (10) , S776-S779
- https://doi.org/10.1139/p68-349
Abstract
The main features of the solar-flare increase in cosmic-ray intensity observed on 28 January 1967 are presented. The flare increase showed no marked anisotropy. It is shown that the onset and decay of this increase can be well accounted for by anisotropic diffusion of particles in a spherically symmetric, inhomogeneous medium with a perfectly absorbing boundary at about 1.3 AU from the sun.Keywords
This publication has 4 references indexed in Scilit:
- Intercomparison of Neutron Monitors During Solar-Flare IncreasesPhysical Review Letters, 1967
- The solar wind velocity and its correlation with cosmic-ray variations and with solar and geomagnetic activityJournal of Geophysical Research, 1963
- Exponential rigidity spectrums for solar-flare cosmic raysJournal of Geophysical Research, 1963
- The cosmic-ray flare effect: 1. Some new methods of analysisJournal of Geophysical Research, 1962