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Two days in the life of AR10486

Published online by Cambridge University Press:  14 March 2005

A.-C. Donea ,
G. Mariş  and
C. A. Lindsey
A.-C. Donea
Affiliation:
Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences, Monash University, Victoria 3800, Australia, Email: alina.donea@sci.monash.edu.au Astronomical Institute of the Romanian Academy, Str. Cutitul de Argint Nr.5, RO-040557, Bucharest, Romania
G. Mariş
Affiliation:
Astronomical Institute of the Romanian Academy, Str. Cutitul de Argint Nr.5, RO-040557, Bucharest, Romania
C. A. Lindsey
Affiliation:
Colorado Research Associates Division, NorthWest Research Associates, Inc., 3380 Mitchell Lane, Boulder, CO 80301, USA.
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Abstract

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Magnetic and acoustic properties of the complex active region AR 486 are analyzed for two consecutive days: October 28 and October 29, 2003 when two large flares of magnitude X17.2 and X10 were produced, respectively. Using the technique of helioseismic holography we detected seismic waves emitted from these flares at 6 mHz. SOHO-MDI white light images, magnetograms, and Dopplergrams are used to study the physics of the acoustic sources.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. 241 - 242
Copyright
© 2004 International Astronomical Union