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Title:
Correlative study of the emission from flares associated with Sun quakes
Authors:
Martínez-Oliveros, J. C.; Donea, A.-C.; Cally, P. S.
Affiliation:
AA(Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences Monash University, VIC 3800, Australia ), AB(Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences Monash University, VIC 3800, Australia ), AC(Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences Monash University, VIC 3800, Australia )
Publication:
Waves & Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology, Proceedings of the International Astronomical Union, IAU Symposium, Volume 247, p. 99-104
Publication Date:
05/2008
Origin:
CUP
Keywords:
Sun: X-rays, Sun: particle acceleration, Sun: helioseismology, Sun: sun quakes, Sun: solar flares
DOI:
10.1017/S1743921308014737
Bibliographic Code:
2008IAUS..247...99M

Abstract

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.
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