THE ANALYSIS OF THE SOLAR X-RAY FLARE ON NOVEMBER 2, 1992
https://doi.org/10.37493/2307-910X.2021.4.29
Abstract
The Yohkoh space solar observatory has been designed to take images of the Sun in the soft X-ray range (10A), with particle energies of ~1 keV. A coronal loop flare occurred on November 2, 1992, which was captured by Yohkoh, which made it possible to record the first time that the top of the coronal loop was periodically pulled up and then closed again. This process is very similar to the way the tail of the Earth's magnetosphere is pulled out during a magnetic substorm. It was also possible to trace the evolution of the loop during a powerful flare.
About the Authors
L. N. Dzhimbeeva
Kalmyk State University
Russian Federation
Russian Federation
G. A. Mankaeva
Kalmyk State University
Russian Federation
Russian Federation
A. Y. Yazlyeva
Kalmyk State University
Russian Federation
Russian Federation
C. S. Akmyradova
Kalmyk State University
Russian Federation
Russian Federation
A. M. Maksatmyradova
Kalmyk State University
Russian Federation
Russian Federation
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Review
For citations:
Dzhimbeeva L.N., Mankaeva G.A., Yazlyeva A.Y., Akmyradova C.S., Maksatmyradova A.M. THE ANALYSIS OF THE SOLAR X-RAY FLARE ON NOVEMBER 2, 1992. Modern Science and Innovations. 2021;(4):249-256. https://doi.org/10.37493/2307-910X.2021.4.29
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