Flare Plasma Diagnostics from X-Ray and Ultraviolet Observations
- Authors: Tsap Y.T.1,2, Motorina G.G.2
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Affiliations:
- Crimean Astrophysical Observatory Scientific Research Institute
- Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
- Issue: Vol 57, No 7 (2017)
- Pages: 916-920
- Section: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/156527
- DOI: https://doi.org/10.1134/S0016793217070246
- ID: 156527
Cite item
Abstract
We compare the measured values of emission measure EM and temperature T of coronal flare plasma following the GOES, RHESSI, and SDO/AIA satellite observations for the events of July 4, 5, and 7, 2012, in the NOAA 11515 active region. We show that the values of EM and T can vary widely (up to one order of magnitude for EM) depending on the technical features of instruments and processing technique. The maximum difference has been found to be between RHESSI and SDO/AIA measurements for temperature and between GOES and SDO/AIA measurements for EM. We discuss the pros and cons of the approaches used and the practical effects of the resulting numerical estimates for EM and T.
About the authors
Yu. T. Tsap
Crimean Astrophysical Observatory Scientific Research Institute; Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
Author for correspondence.
Email: yur_crao@mail.ru
Russian Federation, Nauchny, Crimea, 298409; St. Petersburg, 196140
G. G. Motorina
Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
Email: yur_crao@mail.ru
Russian Federation, St. Petersburg, 196140
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