Solutions to bi-Maxwellian transport equations for radial solar wind beyond 28 Rs
- 31 March 1991
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 39 (3) , 435-451
- https://doi.org/10.1016/0032-0633(91)90005-u
Abstract
No abstract availableKeywords
This publication has 34 references indexed in Scilit:
- Theoretical non-Maxwellian particle velocity distribution functions for spherically symmetric solar wind-like plasma systems and consequences. II - The case of large thermal anisotropy and nine moments description for each speciesThe Astrophysical Journal, 1987
- Numerical investigation of fluid models with full electron and proton thermal conduction equations for the quiet solar windThe Astrophysical Journal, 1984
- Theoretical non-Maxwellian particle velocity distribution functions for spherically symmetric solar wind-like plasma systems and consequencesThe Astrophysical Journal, 1983
- Transport equations for multicomponent anisotropic space plasmas: a reviewPlasma Physics, 1982
- Higher order fluid equations for multicomponent nonequilibrium stellar /plasma/ atmospheres and star clusters. II - Effects of nonzero relative flow velocities and skewing of velocity distribution functionsThe Astrophysical Journal, 1981
- Higher order fluid equations for multicomponent nonequilibrium stellar /plasma/ atmospheres and star clustersThe Astrophysical Journal, 1980
- Hydrodynamic equations for anisotropic plasmas in magnetic fields. II. Transport equations including collisionsPlasma Physics, 1971
- High-latitude plasma transport: The polar windJournal of Geophysical Research, 1969
- Features of plasma transport in the upper atmosphereJournal of Geophysical Research, 1969
- The polar windJournal of Geophysical Research, 1968