On the reality of potential magnetic fields in the solar corona
- 1 October 1978
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 59 (2) , 313-330
- https://doi.org/10.1007/bf00951836
Abstract
No abstract availableKeywords
This publication has 20 references indexed in Scilit:
- Temporal evolution of the equatorialK-coronaSolar Physics, 1977
- Open magnetic structures on the sunThe Astrophysical Journal, 1977
- Coronal emission-line polarization from the statistical equilibrium of magnetic sublevels. I - Fe XIIIThe Astrophysical Journal, 1977
- Physical properties of a polar coronal hole from 2 to 5 solar radiiThe Astrophysical Journal, 1977
- High resolution mapping of the magnetic field of the solar coronaSolar Physics, 1977
- Long-lived coronal structures and recurrent geomagnetic patterns in 1974Planetary and Space Science, 1976
- A new technique for the determination of coronal magnetic fields: A fixed mesh solution to Laplace's equation using line-of-sight boundary conditionsSolar Physics, 1976
- Solar-interplanetary modeling: 3-D solar wind solutions in prescribed non-radial magnetic field geometriesSolar Physics, 1975
- A coronal hole and its identification as the source of a high velocity solar wind streamSolar Physics, 1973
- Polar magnetic fields of the Sun: 1960?1971Solar Physics, 1972