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Role of Magnetic Reconnection in Coronal Heating

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Role of Magnetic Reconnection in Coronal Heating


Dr. Aradhna Sharma



Dr. Aradhna Sharma "Role of Magnetic Reconnection in Coronal Heating" Published in International Journal of Trend in Scientific Research and Development (ijtsrd), ISSN: 2456-6470, Volume-6 | Issue-4, June 2022, pp.731-736, URL: https://www.ijtsrd.com/papers/ijtsrd50179.pdf

The outermost atmosphere of the Sun, called the corona, is some 200 times hotter than the surface of the Sun. The main source of energy for heating the corona is believed to be the magnetic field which dominates the corona. Magnetic reconnection is probably the most important mechanism for releasing magnetic energy and may, therefore, be important for coronal heating or micro-flaring. The best observational examples of reconnection in the corona are thought to be X-ray bright points, which are small-scale brightenings seen randomly throughout the whole corona. Theoretical models can not only explain the key observations relating to bright points, but they can also explain the complex three-dimensional structures often seen in bright points. In these models magnetic neutral points play a significant role as the centres for reconnection both in two and three dimensions.

magnetic, reconnection, corona, heating, dimensional, neural, bright, dimensions


IJTSRD50179
Volume-6 | Issue-4, June 2022
731-736
IJTSRD | www.ijtsrd.com | E-ISSN 2456-6470
Copyright © 2019 by author(s) and International Journal of Trend in Scientific Research and Development Journal. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (CC BY 4.0) (http://creativecommons.org/licenses/by/4.0)

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