Effects of nonâMaxwellian electron velocity distribution functions and nonspherical geometry on minor ions in the solar wind
- 1 February 1987
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 92  (A2) , 1057-1066
- https://doi.org/10.1029/ja092ia02p01057
Abstract
No abstract availableKeywords
This publication has 36 references indexed in Scilit:
- Solar wind carbon, nitrogen and oxygen abundances measured in the Earth's magnetosheath with AMPTE/CCEGeophysical Research Letters, 1986
- Theoretical model of the solar corona during sunspot minimum. II - Dynamic approximationThe Astrophysical Journal, 1985
- Theoretical model of the solar corona during sunspot minimum. I - Quasi-static approximationThe Astrophysical Journal, 1984
- The effect of a non-Maxwellian electron distribution on oxygen and iron ionization balances in the solar coronaThe Astrophysical Journal, 1983
- EUV spectroscopic plasma diagnostics for the solar wind acceleration regionThe Astrophysical Journal, 1982
- The steady global coronaThe Astrophysical Journal, 1982
- Variation of the average âfreezingâinâ temperature of oxygen ions with solar wind speedGeophysical Research Letters, 1980
- Physical properties of a polar coronal hole from 2 to 5 solar radiiThe Astrophysical Journal, 1977
- Electron-impact ionization cross-sections and ionization rate coefficients for atoms and ions from hydrogen to calciumThe European Physical Journal A, 1968
- The State of Ionization of Oxygen in the Solar WindThe Astrophysical Journal, 1968