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Slight Disappearance of Prominence Plasma to the Solar Corona

Published online by Cambridge University Press:  19 July 2016

V. Rusin ,
V. Dermendjiev ,
M. Rybansky  and
G. Buyukliev
V. Rusin
Affiliation:
Astronomical Institute Slovak Academy of Sciences 059 60 Tatranska Lomnica Czechoslovakia Department of Astronomy and NAO 72 Lenin Blvd. 1784 Sofia Bulgaria
V. Dermendjiev
Affiliation:
Astronomical Institute Slovak Academy of Sciences 059 60 Tatranska Lomnica Czechoslovakia Department of Astronomy and NAO 72 Lenin Blvd. 1784 Sofia Bulgaria
M. Rybansky
Affiliation:
Astronomical Institute Slovak Academy of Sciences 059 60 Tatranska Lomnica Czechoslovakia Department of Astronomy and NAO 72 Lenin Blvd. 1784 Sofia Bulgaria
G. Buyukliev
Affiliation:
Astronomical Institute Slovak Academy of Sciences 059 60 Tatranska Lomnica Czechoslovakia Department of Astronomy and NAO 72 Lenin Blvd. 1784 Sofia Bulgaria

Extract

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The problem of prominences-corona relationship is relativelly old. Already in 1931 Lockyer [1] showed that there is a close relation between prominences distribution and the form of white-light corona. However, this problem is still debatable and poses a number of controversial questions. One of them is the question of the energy and mass exchange between prominences and the ambient corona. It is generally assumed that the mass balance exists between the corona and prominences, but unambiguous observational proofs for prominences-corona plasma exchange are very rare. There are little data [2-4], as well, that could be used to address the problem of slight plasma flows from prominences to the corona.

Type
VII. Magnetic Reconnection and Coronal Evolution
Information
Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 347 - 349
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

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