Hydrodynamic models of the solar corona
- 1 November 1962
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 67 (12) , 4577-4584
- https://doi.org/10.1029/jz067i012p04577
Abstract
No abstract availableKeywords
This publication has 15 references indexed in Scilit:
- The Heating of the Solar Chromosphere, Plages, and Corona by Magnetohydrodynamic Waves.The Astrophysical Journal, 1961
- Interplanetary Gas. III. a Hydrodynamic Model of the Corona.The Astrophysical Journal, 1961
- The Hydrodynamic Theory of Solar Corpuscular Radiation and Stellar Winds.The Astrophysical Journal, 1960
- The Hydrodynamic Treatment of the Expanding Solar Corona.The Astrophysical Journal, 1960
- The Telluric Hydrogen Corona.The Astrophysical Journal, 1960
- Interplanetary Gas.II. Expansion of a Model Solar Corona.The Astrophysical Journal, 1960
- Distribution of Density in a Planetary ExospherePhysics of Fluids, 1959
- Dynamics of the Interplanetary Gas and Magnetic Fields.The Astrophysical Journal, 1958
- Notes on the solar corona and the terrestrial ionosphereSmithsonian Contributions to Astrophysics, 1957
- The Boltzmann equation an d the one-fluid hydromagnetic equations in the absence of particle collisionsProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1956