Effects of rapidly diverging flow, heat addition, and momentum addition in the solar wind and stellar winds
- 1 January 1977
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 82 (1) , 23-35
- https://doi.org/10.1029/ja082i001p00023
Abstract
No abstract availableKeywords
This publication has 35 references indexed in Scilit:
- The subsonic structure of radiatively driven winds of early-type starsThe Astrophysical Journal, 1975
- Plasma processes in the expansion of the solar wind and in the interplanetary mediumReviews of Geophysics, 1975
- Theoretical Studies of the Large-Scale Behavior of the Solar WindPublished by Elsevier ,1975
- Radiation-driven winds in Of starsThe Astrophysical Journal, 1975
- The profile and polarization of the coronal L? lineSolar Physics, 1974
- Optically Thin Stellar Winds in Early-Type StarsThe Astrophysical Journal, 1973
- On the Energy Transport in Stellar WindsThe Astrophysical Journal, 1971
- Solar wind ions:56Fe+8to56Fe+12,28Si+7,28Si+8,28Si+9, and16O+6Journal of Geophysical Research, 1970
- Solar wind and interplanetary magnetic fieldReviews of Geophysics, 1967
- On the Solutions of Parker's Hydrodynamic Theory of Solar and Stellar Winds.The Astrophysical Journal, 1965