A two‐fluid solar wind model with Alfven waves: Parameter study and application to observations
- 1 March 1986
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 91 (A3) , 2950-2960
- https://doi.org/10.1029/ja091ia03p02950
Abstract
No abstract availableKeywords
This publication has 33 references indexed in Scilit:
- Fast-mode magnetohydrodynamic waves in coronal holes and the solar windThe Astrophysical Journal, 1984
- Analysis of coronal H I Lyman alpha measurements from a rocket flight on 1979 April 13The Astrophysical Journal, 1982
- Electron heating by fast mode magnetohydrodynamic waves in the solar wind emanating from coronal holesThe Astrophysical Journal, 1982
- Measurements of coronal kinetic temperatures from 1.5 to 3 solar radiiThe Astrophysical Journal, 1980
- The dynamical properties of the solar corona from intensities and line widths of EUV forbidden lines of SI VIII, Fe XI, and Fe XIIThe Astrophysical Journal, 1979
- Signatures of solar wind latitudinal structure in interplanetary Lyman-alpha emissions - Mariner 10 observationsThe Astrophysical Journal, 1979
- ALFVtN Waves in a Two-Fluid Model of the Solar WindThe Astrophysical Journal, 1973
- ALFVÉNIC Wave Pressures and the Solar WindThe Astrophysical Journal, 1971
- Calculations of Ionization Equilibria for Oxygen, Neon, Silicon, and IronThe Astrophysical Journal, 1969
- Two-Fluid Model of the Solar WindPhysical Review Letters, 1966