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Sunspots and magnetohydrodynamic flows
Published online by Cambridge University Press: 14 August 2015
Abstract
Theoretical techniques are developed to study compressible, steady-state, magnetically aligned gas flows in sunspot regions. The flows are adiabatic and occur in a known streamline configuration. The non-linear parabolic partial differential equation describing the flow reduces to an ordinary linear differential equation. The solutions are briefly discussed.
- Type
- Part II: Theoretical Aspects
- Information
- Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 142 - 147
- Copyright
- Copyright © Reidel 1968