Vol. 5 (04) pp. 349-351 DOI: 10.21474/IJAR01/3818

MAGNETIC RECONNECTION MODEL FOR CORONAL HEATING.

  • Department of Applied Science, Nanhi Pari Seemant Engineering Institute Pithoragarh, Uttarakhand.
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Abstract

Sun is a most important star in our universe. The solar corona is the strange place. Its heating is highly complex with many different facts in Astrophysics. It is likely that different heating mechanism is at work in solar corona. Reconnection is a fundamental process in plasma. In this paper I describe Magnetic reconnection model for solar coronal heating.

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References

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How to Cite This Article

Chandra Mohan S. Negi. (2017); MAGNETIC RECONNECTION MODEL FOR CORONAL HEATING., Int. J. of Adv. Res., 5 (04), 349-351, ISSN 2320-5407. DOI: https://doi.org/10.21474/IJAR01/3818

Corresponding Author

CHANDRA MOHAN SINGH NEGI
UTTARAKHAND TECHNICAL UNIVERSITY,DEHRADUN
Creative Commons Attribution 4.0 This work is licensed under a Creative Commons Attribution 4.0 International License.