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Energy Balance in Prominence-Corona Transition Regions

Published online by Cambridge University Press:  19 July 2016

C. Chiuderi  and
F. Chiuderi Drago
C. Chiuderi
Affiliation:
Department of Astronomy and Space Science, University of Florence Largo Enrico Fermi 5 50125 Florence, Italy
F. Chiuderi Drago
Affiliation:
Department of Astronomy and Space Science, University of Florence Largo Enrico Fermi 5 50125 Florence, Italy

Extract

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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

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