Changes in the energy spectrum of anomalous oxygen during 1977–1985
- 1 March 1986
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 91 (A3) , 2896-2902
- https://doi.org/10.1029/ja091ia03p02896
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- Evidence that the anomalous cosmic-ray component is singly ionizedThe Astrophysical Journal, 1984
- Elemental composition of solar energetic particlesThe Astrophysical Journal, 1984
- Cosmic ray drift, shock wave acceleration, and the anomalous component of cosmic raysThe Astrophysical Journal, 1981
- On the charge state of the anomalous oxygen componentGeophysical Research Letters, 1980
- Observed distribution functions of H, He, C, O, and Fe in corotating energetic particle streams - Implications for interplanetary acceleration and propagationThe Astrophysical Journal, 1979
- Observations of galactic cosmic-ray energy spectra between 1 and 9 AUThe Astrophysical Journal, 1977
- An Interpretation of the Observed Oxygen and Nitrogen Enhancements in Low-Energy Cosmic RaysThe Astrophysical Journal, 1974
- The Anomalous Abundance of Cosmic-Ray Nitrogen and Oxygen Nuclei at Low EnergiesThe Astrophysical Journal, 1974
- Differential Energy Spectra of Low-Energy (<8.5 MeV per Nucleon) Heavy Cosmic Rays during Solar Quiet TimesPhysical Review Letters, 1973
- A New Test for Solar Modulation Theory: the 1972 May-July Low-Energy Galactic Cosmic-Ray Proton and Helium SpectraThe Astrophysical Journal, 1973