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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
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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Aschwanden, M.: 2004, Astrophys. J. 608, 554CrossRefGoogle Scholar
Bastian, T.S., Benz, A.O, Gary, D.E: 1998, Annu. Rev. Astron. Astrophys., 36, 131CrossRefGoogle Scholar
Besliu-Ionescu, D., Donea, A.-C., Cally, P. S. and Lindsey, C.: 2006, “Seismic Radiation from M-class Solar Flares,” Beyond the Spherical Sun: a new era in helio-and asteroseismology, Proc. of SOHO-18/GONG-2006/HELAS I ed. Fleck, B. (ESA Public.), CDROM, pp.67.1.Google Scholar
Ding, M. D., Liu, Y., Yeh, C.-T., Li, J. P.: 2003, Astron. Astrophys. 403, 1151CrossRefGoogle Scholar
Donea, A.-C., Beşliu-Ionescu, D., Lindsey, C. & Zharkova, V. V. 2006, Solar Phys. 239, 113CrossRefGoogle Scholar
Donea, A.-C., Braun, D. C & Lindsey, C., 1999, Astrophys. J. 513, L143CrossRefGoogle Scholar
Donea, A.-C., & Lindsey, C., 2005 Astrophys. J. 630, 1168.CrossRefGoogle Scholar
Grechnev, V.: 2003, Solar Phys. 213, 103CrossRefGoogle Scholar
Kosovichev, A.G., Zharkova, V.V., 1998, Nature 393, 317CrossRefGoogle Scholar
Kosovichev, A.G., 2006, Solar Phys. 238, 1CrossRefGoogle Scholar
Li, J.P., Ding, D. & Liu, Y.: 2005, Solar Phys. 229, 115CrossRefGoogle Scholar
Lindsey, C., & Braun, D. C., 2000, Solar Phys. 192, 261.CrossRefGoogle Scholar
Liu, Y., Ding, M. D., and Fang, C: 2001, Astronom. J. 563, L169CrossRefGoogle Scholar
Martinez-Oliveros, J.C., Moradi, H., Besliu-Ionescu, D., Donea, A.-C, Cally, P., Lindsey, C., 2007a, Solar Phys. 245, 121CrossRefGoogle Scholar
Martinez-Oliveros, J.C., Moradi, H. D., Donea, A.-C 2007b, Solar Phys. submitted.Google Scholar
Moradi, H.; Donea, A.-C.; Lindsey, C.; Besliu-Ionescu, D.; Cally, P. S., 2007, Mon. Not. Roy. Astron. Soc. 374, 3, 1155CrossRefGoogle Scholar
Rajaguru, S. P., Birch, A. C., Duvall, T. L. Jr., Thompson, M. J., Zhao, J.: 2006, Astrophys. J. 646, 543CrossRefGoogle Scholar
Uddin, W., Jain, R., Yoshimura, K., Chandra, R., Sakao, T., Kosugi, T., Joshi, A., Despande, M. R.: 2004, Solar Phys. 225, 325CrossRefGoogle Scholar
Zharkova, V.V., & Kobylinskii, V.A., 1993, Solar Phys. 143, 249.CrossRefGoogle Scholar
Zharkova, V.V., & Zharkov, S.I., 1993, Astrophys. J. 664, 573CrossRefGoogle Scholar