Flare Plasma Diagnostics from X-Ray and Ultraviolet Observations


Cite item

Full Text

Open Access Open Access
Restricted Access Access granted
Restricted Access Subscription Access

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

Supplementary files

Supplementary Files
Action
1. JATS XML

Copyright (c) 2017 Pleiades Publishing, Ltd.