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Gyroscopic waves in the base of the solar corona: A model and possible observational manifestationsA linear model for gyroscopic waves in the base of the solar corona is proposed. The purpose was to point out possible observational manifestations of the phenomenon. According to the model, these waves move slowly around the sun along heliolatitude circles. The fact that the red line corona is fainter on the solar side facing the apex and north-south and east-west asymmetries of the red coronal emission line could be interpreted as a possible observational manifestation of the gyroscopic wave phenomenon in the coronal base.
Document ID
19990028130
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
Pisanko, Y. V.
(Institute of Applied Geophysics Moscow USSR)
Tritakis, V. P.
(Academy of Athens Greece)
Paliatsos, A. G.
(Piraeus Univ. Piraeus Greece)
Date Acquired
August 19, 2013
Publication Date
September 1, 1997
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
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