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C-1.4 class flare and an associated peculiar coronal jet

Published online by Cambridge University Press:  27 November 2018

Ritika Solanki ,
Abhishek K. Srivastava  and
B. N. Dwivedi
Ritika Solanki
Affiliation:
Department of Physics, Indian Institute of Technology (BHU), Varanasi - 221005, India. email: [email protected], [email protected]
Abhishek K. Srivastava
Affiliation:
Department of Physics, Indian Institute of Technology (BHU), Varanasi - 221005, India. email: [email protected], [email protected]
B. N. Dwivedi
Affiliation:
Department of Physics, Indian Institute of Technology (BHU), Varanasi - 221005, India. email: [email protected], [email protected]
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Abstract

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Using HINODE/XRT, GOES, SDO/AIA observations, we study a compact C-1.4 class flare outside a major sunspot of AR 12178 on 4 October 2014. This flare is associated with a peculiar coronal jet, which is erupted in two stages in the overlying corona above the compact flaring region. At the time of flare maximum, the first stage of the jet eruption occurs above the flare energy release site, and thereafter in the second stage its magneto-plasma system interacts with the overlying distinct magnetic field domain in its vicinity to build further the typical jet plasma column.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S340: Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles , February 2018 , pp. 193 - 195
Copyright
Copyright © International Astronomical Union 2018 

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