Inhibition of conductive heat flow by magnetic constriction in the corona and transition region: Dependence on the shape of the constriction
- 1 September 1985
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 99 (1) , 79-99
- https://doi.org/10.1007/bf00157300
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Chromosphere-corona transition region models with magnetic field and fluid flowThe Astrophysical Journal, 1981
- The evolution of active region loop plasmaThe Astrophysical Journal, 1980
- The energy balance and pressure in the solar transition zone for network and active region featuresThe Astrophysical Journal, 1979
- Recent Advances in Coronal PhysicsAnnual Review of Astronomy and Astrophysics, 1978
- Dynamics of the quiescent solar coronaThe Astrophysical Journal, 1978
- Mass and Energy Flow in the Solar Chromosphere and CoronaAnnual Review of Astronomy and Astrophysics, 1977
- Influence of magnetic field structure on the conduction cooling of flare loopsSolar Physics, 1976
- 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
- Structure of the chromosphere-corona transition regionSolar Physics, 1972
- Magnetic fields and the temperature structure of the chromosphere-corona interfaceSolar Physics, 1968