A fast solar wind model with anisotropic proton temperature
- 3 January 1997
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 102 (A7) , 14661-14676
- https://doi.org/10.1029/97ja01040
Abstract
No abstract availableKeywords
This publication has 43 references indexed in Scilit:
- Measurement of Hydrogen Velocity Distributions in the Extended Solar CoronaThe Astrophysical Journal, 1996
- Physical Properties of Polar Coronal Rays and Holes as Observed with the Spartan 201-01 CoronagraphThe Astrophysical Journal, 1995
- Flow properties of the solar wind derived from a two‐fluid model with constraints from white light and in situ interplanetary observationsGeophysical Research Letters, 1995
- Ion and electron suprathermal tail strengths in the transition region: Support for the velocity filtration model of the coronaThe Astrophysical Journal, 1994
- Acceleration and heating of two-fluid solar wind by Alfven wavesThe Astrophysical Journal, 1994
- How reliable are coronal hole temperatures deduced from observations?The Astrophysical Journal, 1993
- Effect of coupled electron-proton thermal conductivities on the two-fluid solutions for the quiet solar windThe Astrophysical Journal, 1988
- A time-dependent two-fluid model with thermal conduction for the solar windThe Astrophysical Journal, 1979
- Heat Conductivity, Plasma Instabilities, and Radio-Star - Lations in the Solar WindThe Astrophysical Journal, 1973
- Two-Fluid Model of the Solar WindThe Astrophysical Journal, 1968