Interplanetary diffusion model for the time behavior of intensity in a solar cosmic ray event
- 1 July 1965
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 70 (13), 2943-2960
- https://doi.org/10.1029/jz070i013p02943
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- A survey of electronsE> 40 kev beyond 5 Earth radii with Explorer 14Journal of Geophysical Research, 1965
- Continual Acceleration of Solar Protons in the MeV RangePhysical Review Letters, 1965
- A diffusive model for the initial phase of a solar proton eventJournal of Geophysical Research, 1964
- The scattering of charged particles by magnetic irregularitiesJournal of Geophysical Research, 1964
- The time variations of solar cosmic rays during the September 3, 1960, eventJournal of Geophysical Research, 1963
- Simultaneous balloon observations at Fort Churchill and Minneapolis during the solar cosmic ray events of July 1961Journal of Geophysical Research, 1963
- Primary Cosmic Ray and Solar Protons. IIPhysical Review B, 1963
- Explorer 12 observations of solar cosmic rays and energetic storm particles after the solar flare of September 28, 1961Journal of Geophysical Research, 1962
- Balloon measurement of solar cosmic rays at Fort Churchill, Canada, during July 1959Journal of Geophysical Research, 1961
- The time variations of solar cosmic rays during July 1959 at MinneapolisJournal of Geophysical Research, 1961