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Analysis of quasi-periodic oscillations of position and brightness of details of the radio sources of the solar active regions based on observations made with the radio heliograph Nobeyama

Published online by Cambridge University Press:  14 March 2005

G.B. Gelfreikh ,
K. Shibasaki ,
E.Yu. Nagovitsyna  and
Yu.A. Nagovitsyn
G.B. Gelfreikh
Affiliation:
Central astronomical observatory at Pulkovo of RAS, St.-Petersburg, Russia, email: gbg@GG1623.spb.edu
K. Shibasaki
Affiliation:
Nobeyama solar radio observatory, Japan
E.Yu. Nagovitsyna
Affiliation:
Central astronomical observatory at Pulkovo of RAS, St.-Petersburg, Russia, email: gbg@GG1623.spb.edu
Yu.A. Nagovitsyn
Affiliation:
Central astronomical observatory at Pulkovo of RAS, St.-Petersburg, Russia, email: gbg@GG1623.spb.edu
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Abstract

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As based on analysis of radio maps at the wavelength of 1.76 cm obtained from observations at the radio heliograph Nobeyama the parameters of oscillation processes in solar active regions were studied. As a technique for data processing wavelet analysis was used. The inherent periodicity in oscillations submits the existence of a resonance structure for some kinds of MHD waves in the plasma of the solar atmosphere.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. 245 - 246
Copyright
© 2004 International Astronomical Union