Detailed directional and temporal properties of solar energetic particles associated with propagating interplanetary shock waves
Authors:
- Sidney SingerSSSidney Singer
- Michael D. MontgomeryMMMichael D. Montgomery
- 1 October 1971
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 76 (28) , 6628-6642
Abstract
No abstract availableKeywords
This publication has 22 references indexed in Scilit:
- Increases in the low-energy cosmic ray intensity at the front of propagating interplanetary shock wavesJournal of Geophysical Research, 1971
- Proton fluxes at 300 kev associated with propagating interplanetary shock wavesJournal of Geophysical Research, 1970
- A comparison of energetic storm protons to halo protonsSolar Physics, 1969
- Solar flare injection and propagation of low-energy protons and electrons in the event of 7?9 July, 1966Solar Physics, 1968
- Cosmic Rays in the Interplanetary MediumThe Astrophysical Journal, 1967
- Discontinuities in the solar windSpace Science Reviews, 1966
- a Model of Fermi Acceleration at Shock Fronts with an Application to the Earth's Bow ShockThe Astrophysical Journal, 1966
- Vela Satellite Measurements of Particles in the Solar Wind and the Distant Geomagnetosphere1966
- Increases in intensity of solar cosmic rays before sudden commencements of geomagnetic stormsJournal of Geophysical Research, 1963
- Explorer 12 observations of solar cosmic rays and energetic storm particles after the solar flare of September 28, 1961Journal of Geophysical Research, 1962