Article contents
Hydromagnetic Structure at the Boundary of a Supergranule
Published online by Cambridge University Press: 25 April 2016
Extract
We shall examine the question of whether the concentration of magnetic field, the downward motion and the temperature excess observed at the boundaries of supergranules can be interpreted consistently in terms of a steady flow along the magnetic lines of force. Before doing so, however, we shall first consider the development of the magnetic configuration driven by a supergranular convection overshooting into the photosphere.
- Type
- Contributions
- Information
- Publications of the Astronomical Society of Australia , Volume 2 , Issue 1 , July 1971 , pp. 54 - 55
- Copyright
- Copyright © Astronomical Society of Australia 1971
References
- 3
- Cited by