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Transfer of energy within coronal bright points according to the observation in optical spectra and microwave

Published online by Cambridge University Press:  14 March 2005

D. V. Prosovetsky  and
L. K. Kashapova
D. V. Prosovetsky
Affiliation:
Institute of Solar-Terrestrial Physics SB RAS, Irkutsk, Russia, email: proso@iszf.irk.ru
L. K. Kashapova
Affiliation:
Institute of Solar-Terrestrial Physics SB RAS, Irkutsk, Russia, email: proso@iszf.irk.ru
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Abstract

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The paper is devoted to the coronal bright points. We carried out the analysis of the simultaneous observations in IR He $\lambda$10830 Å and microwaves at 5.2 and 1.76 cm. It was obtained that microwave sources correspond to the dark points in IR He $\lambda$10830 Å with line-of-sight velocities directed from a observer. The possible mechanism of the energy transport within the bright points are suggested.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. 479 - 480
Copyright
© 2004 International Astronomical Union