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Investigation of wave characteristics by red coronal line observations

Published online by Cambridge University Press:  14 March 2005

S. I. Molodykh  and
N. F. Tyagun
S. I. Molodykh
Affiliation:
Institute of Solar-Terrestrial Physics SB RAS, 664033, Irkutsk, P.O.Box 4026, Russia email: sim@iszf.irk.ru Present address: Institute of Solar-Terrestrial Physics, 664033, Irkutsk, P.O.Box 4026, Russia.
N. F. Tyagun
Affiliation:
Institute of Solar-Terrestrial Physics SB RAS, 664033, Irkutsk, P.O.Box 4026, Russia email: sim@iszf.irk.ru
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Abstract

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This paper presents the results of the active region observations in red coronal line ($\lambda = 6374 \stackrel{\circ}{\rm A}$). The analysis was made of the dependence of the profile parameters of the red coronal line on the exposition value.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 649 - 650
Copyright
© 2004 International Astronomical Union