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On the Possibility of Identifying Coronal Holes on Synoptic Maps of the Green Corona

Published online by Cambridge University Press:  14 August 2015

V. Letfus ,
L. Kulčár  and
J. SýKora
V. Letfus
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, 251 65 Ondřejov, Czechoslovakia
L. Kulčár
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, Skalnaté Pleso, 059 60 Tatranská Lomnica, Czechoslovakia
J. SýKora
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, Skalnaté Pleso, 059 60 Tatranská Lomnica, Czechoslovakia

Extract

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The coronal holes of the Skylab period are treated to identify them with the low-brightness regions in our synoptic maps of the λ 530.3 nm emission corona. Possibilities and difficulties of this identification are discussed.

Type
Part I. The Life History of Coronal Structures and Fields
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 49 - 53
Copyright
Copyright © Reidel 1980 

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