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Energy Balance in Prominence-Corona Transition Regions
Published online by Cambridge University Press: 19 July 2016
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Prominences are sheets of cold (< 104 K) plasma totally imbedded in the hot (> 106 K) coronal plasma. A Prominence-Corona Transition Region (PCTR) is therefore present all around it.
- Type
- VII. Magnetic Reconnection and Coronal Evolution
- Information
- Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 325 - 329
- Copyright
- Copyright © Kluwer 1990
References
REFERENCES
Engvold, O.: 1989, “Dynamic and Structure of Quiescent Solar Prominences”, Ed. Priest, E. R.
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Leroy, J.L.: 1989, “Dynamic and Structure of Quiescent Solar Promineces”, Ed. Priest, E. R.
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Schmahl, E. and Orral, F.: 1986, “Coronal and Prominences Plasmas”, NASA Conf. Pub.
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