RHESSI observations of long-duration flares with long-lasting X-ray loop-top sources
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201016176/pdf
Reference50 articles.
1. On the Photometric Accuracy of RHESSI Imaging and Spectrosocopy
2. Carmichael, H. 1963, AAS-NASA Symposium on the Physics of Solar Flares, NASA SP-30, 451
3. RHESSI LINE AND CONTINUUM OBSERVATIONS OF SUPER-HOT FLARE PLASMA
4. Evidence for Chromospheric Evaporation in the Late Gradual Flare Phase from [ITAL]SOHO[/ITAL]/CDS Observations
5. EIT: Extreme-ultraviolet Imaging Telescope for the SOHO mission
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1. Plasma dynamics in the flaring loop observed by RHESSI;Astronomy & Astrophysics;2021-12-22
2. Multiwavelength Analysis of the Kinematics of a Long Duration Flare-CME Event on 27 January 2012;Solar Physics;2020-09
3. Quasi-periodic pulsations in a solar flare with an unusual phase shift;Monthly Notices of the Royal Astronomical Society;2018-12-27
4. On the fine structure of solar flare X-ray loop top sources;Proceedings of the International Astronomical Union;2015-08
5. TEMPORAL VARIATIONS OF X-RAY SOLAR FLARE LOOPS: LENGTH, CORPULENCE, POSITION, TEMPERATURE, PLASMA PRESSURE, AND SPECTRA;The Astrophysical Journal;2013-03-11
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