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Correlative study of the emission from flares associated with Sun quakes

Published online by Cambridge University Press:  01 September 2007

J. C. Martínez-Oliveros ,
A.-C. Donea  and
P. S. Cally
J. C. Martínez-Oliveros
Affiliation:
Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences Monash University, VIC 3800, Australia email: Juan.Oliveros@sci.monash.edu.au
A.-C. Donea
Affiliation:
Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences Monash University, VIC 3800, Australia email: Juan.Oliveros@sci.monash.edu.au
P. S. Cally
Affiliation:
Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences Monash University, VIC 3800, Australia email: Juan.Oliveros@sci.monash.edu.au
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Abstract

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Multi-wavelength studies of energetic solar flares with seismic emissions have revealed interesting common features that may help us to identify the correlations of flare signatures from the inner to the outer solar atmosphere and, to develop diagnostic techniques to aid in the sun quake detection. In our study, we make use the relation between the microwave and the hard X-ray emissions associated with such flares to propose a scenario for the ignition of seismic transients from flares. We explore the mechanisms of energy transport to the photosphere, such us back-warming or direct particle impacts.

Keywords

Sun: X-raysSun: particle accelerationSun: helioseismologySun: sun quakesSun: solar flares
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S247: Waves & Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology , September 2007 , pp. 99 - 104
Copyright
Copyright © International Astronomical Union 2008

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