Mechanisms for the rigid rotation of coronal holes
- 1 September 1988
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 117 (2) , 359-389
- https://doi.org/10.1007/bf00147253
Abstract
No abstract availableKeywords
This publication has 51 references indexed in Scilit:
- The quasi-rigid rotation of coronal magnetic fieldsThe Astrophysical Journal, 1988
- The origin of rigidly rotating magnetic field patterns on the sunThe Astrophysical Journal, 1987
- Recent Studies of Magnetic CanopiesAustralian Journal of Physics, 1985
- Rotational characteristics of the white-light solar corona 1965-1983The Astrophysical Journal, 1984
- Magnetic rotation of the solar photosphereThe Astrophysical Journal, 1983
- The influence of differential rotation on the equatorial component of the sun's magnetic dipole fieldThe Astrophysical Journal, 1981
- A Discussion on the physics of the solar atmosphere - A magnetic model of the solar transition regionPhilosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1976
- Solar rotation as marked by extreme-ultraviolet coronal holesThe Astrophysical Journal, 1975
- The reconnection of magnetic field lines in the solar coronaThe Astrophysical Journal, 1975
- Transport of Magnetic Fields on the Sun.The Astrophysical Journal, 1964