The magnetic and thermodynamical structure of a coronal hole
- 1 June 1985
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 97 (2) , 251-266
- https://doi.org/10.1007/bf00165989
Abstract
No abstract availableKeywords
This publication has 23 references indexed in Scilit:
- Theoretical model of the solar corona during sunspot minimum. I - Quasi-static approximationThe Astrophysical Journal, 1984
- Combined effect of potential and nonpotential magnetic fields on equilibrium in stellar atmospheresThe Astrophysical Journal, 1984
- Magnetohydrostatic model of solar faculaeThe Astrophysical Journal, 1983
- On the magnetic and thermodynamic consequences of the return-flux sunspot modelThe Astrophysical Journal, 1982
- The magnetohydrostatic atmosphere around a gravitating bodyThe Astrophysical Journal, 1982
- Solar polar coronal hole - A mathematical simulationThe Astrophysical Journal, 1977
- Physical properties of a polar coronal hole from 2 to 5 solar radiiThe Astrophysical Journal, 1977
- A coronal hole and its identification as the source of a high velocity solar wind streamSolar Physics, 1973
- Coronal electron density maps for 7 March, 1970, derived from Mgx ?625 spectroheliogramsSolar Physics, 1971
- Gas-magnetic field interactions in the solar coronaSolar Physics, 1971