Interplanetary ions during an energetic storm particle event: The distribution function from solar wind thermal energies to 1.6 MeV
- 1 February 1981
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 86 (A2) , 547-554
- https://doi.org/10.1029/ja086ia02p00547
Abstract
No abstract availableKeywords
This publication has 40 references indexed in Scilit:
- Acceleration theory for 5–40 keV ions at interplanetary shocksAdvances In Space Research, 1981
- Shock acceleration of energetic particles in corotating interaction regions in the solar windThe Astrophysical Journal, 1980
- Singly‐ionized helium in the driver gas of an interplanetary shock waveGeophysical Research Letters, 1980
- Characteristics of the spectra of protons and alpha particles in recurrent events at 1 AuGeophysical Research Letters, 1979
- Observed distribution functions of H, He, C, O, and Fe in corotating energetic particle streams - Implications for interplanetary acceleration and propagationThe Astrophysical Journal, 1979
- Evidence for interplanetary acceleration of nucleons in corotating interaction regionsThe Astrophysical Journal, 1976
- Observations of interaction regions and corotating shocks between one and five AU: Pioneers 10 and 11Geophysical Research Letters, 1976
- The interplanetary acceleration of energetic nucleonsThe Astrophysical Journal, 1976
- Post-shock spikes: A new feature of proton and alpha enhancements associated with an interplanetary shock waveGeophysical Research Letters, 1974
- Electrons and protons in long-lived streams of energetic solar particlesSolar Physics, 1969