Interplanetary gas X. Coronal temperatures, energy deposition, and the solar wind
- 30 April 1965
- Vol. 4 (1) , 19-36
- https://doi.org/10.1016/0019-1035(65)90014-x
Abstract
No abstract availableKeywords
This publication has 32 references indexed in Scilit:
- A Gas-Dynamic Model of the Outer Solar Atmosphere.The Astrophysical Journal, 1964
- Spectroscopic Limitation on Coronal Heating Mechanisms.The Astrophysical Journal, 1963
- Coronal Temperature Gradient and the Solar Wind.The Astrophysical Journal, 1963
- Observations of the Zodiacal Light from a Very High Altitude Station: II. Electron Densities in Interplanetarry SpaceMonthly Notices of the Royal Astronomical Society, 1961
- Distribution of Matter with Temperature in the Emission Corona.The Astrophysical Journal, 1959
- An Examination of the Observational Evidence for the Accretion Theory of the Solar CoronaMonthly Notices of the Royal Astronomical Society, 1956
- The Physical Condition of the Solar CoronaReports on Progress in Physics, 1954
- Interpretation of Electron Densities from Corona BrightnessMonthly Notices of the Royal Astronomical Society, 1947
- Granulation, Magneto-Hydrodynamic Waves, and the Heating of the Solar CoronaMonthly Notices of the Royal Astronomical Society, 1947
- Zur Deutung der chromosph rischen Turbulenz und des Exzesses der UV-Strahlung der SonneThe Science of Nature, 1946