THE ANALYSIS OF THE SOLAR X-RAY FLARE ON NOVEMBER 2, 1992
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...
Saved in:
Main Authors: | L. N. Dzhimbeeva, G. A. Mankaeva, A. Y. Yazlyeva, C. S. Akmyradova, A. M. Maksatmyradova |
---|---|
Format: | Article |
Language: | Russian |
Published: |
North-Caucasus Federal University
2022-08-01
|
Series: | Современная наука и инновации |
Subjects: | |
Online Access: | https://msi.elpub.ru/jour/article/view/496 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The Payload Design of the CUbesat Solar Polarimeter (CUSP), for Space Weather and Solar Flares X-Ray Polarimetry
by: Giovanni Lombardi, et al.
Published: (2025-03-01) -
SPECTRAL ESTIMATION OF TIME SERIES
by: L. N. Dzhimbeeva, et al.
Published: (2022-08-01) -
Towards a quantitative theory for transmission X-ray microscopy
by: James G. McNally, et al.
Published: (2025-07-01) -
The First AGILE Solar Flare Catalog
by: A. Ursi, et al.
Published: (2023-01-01) -
High-resolution Observations of an X6.4 Solar Flare in the Mid-infrared
by: Xu Yang, et al.
Published: (2025-01-01)