The expansion of a low-density solar corona: A one-fluid model with magnetically modified thermal conductivity
- 1 September 1974
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 79 (25) , 3711-3716
- https://doi.org/10.1029/ja079i025p03711
Abstract
No abstract availableKeywords
This publication has 20 references indexed in Scilit:
- On the Thermal Conductivity of the Quiet Solar-Wind Plasma and ConsequencesThe Astrophysical Journal, 1973
- A coronal hole and its identification as the source of a high velocity solar wind streamSolar Physics, 1973
- Coronal density and temperature gradientsSolar Physics, 1973
- Coronal holesSolar Physics, 1972
- Solar-wind properties at the Earth as Predicted by One-Fluid ModelsJournal of Geophysical Research, 1972
- History and BackgroundPublished by Springer Nature ,1972
- A New Type of Supersonic Solution for the Inviscid Equations of the Solar WindThe Astrophysical Journal, 1971
- The Theory of Stellar Winds and Related FlowsAnnual Review of Astronomy and Astrophysics, 1970
- Interplanetary Gas. XVI. a Calculation of the Angular Momentum of the Solar WindThe Astrophysical Journal, 1969
- Interplanetary gas XI. An exospheric model of the solar windIcarus, 1966