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Energy distribution of solar flare events

Published online by Cambridge University Press:  27 November 2018

S. Sen
Affiliation:
Indian Institute of Astrophysics Sarjapur Road, Koramangala, Bangalore, 560034, India email: [email protected]
A. Mangalam
Affiliation:
Indian Institute of Astrophysics Sarjapur Road, Koramangala, Bangalore, 560034, India [email protected]
R. Ramesh
Affiliation:
Indian Institute of Astrophysics Sarjapur Road, Koramangala, Bangalore, 560034, India [email protected]
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Abstract

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The coronal field typically reorganizes itself to attain a force-free field configuration. We have evaluated the power law index of the energy distribution f(E) = f0E−α by using a model of relaxation incorporating different profile functions of winding number distribution f(w) based on braided topologies. We study the radio signatures that occur in the solar corona using the radio data obtained from the Gauribidanur Radio Observatory (IIA) and extract the power law index by using the Statistic-sensitive nonlinear iterative peak clipping (SNIP) algorithm. We see that the power law index obtained from the model is in good agreement with the calculated value from the radio data observation.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Berger, A. & Asgari-Targhi, , 2009, ApJ, 705, 347Google Scholar
Mangalam, A. & Prasad, A., 2018, AdSpR, 61, 738Google Scholar
Prasad, A. & Mangalam, A., 2013, ASInC, 10, 51Google Scholar
Prasad, , et al. 2014, ApJ, 786, 81Google Scholar
Ramesh, , et al. 2013, ApJ, 762, 89Google Scholar
Ramesh, R., 2011, ASI Conf. Ser., 2, 55Google Scholar
Tomoyori, , et al. 2015, J. Phys.: Conf. Ser., 664, 072049Google Scholar