http://arxiv.org/abs/1604.01926
We explore the temporal evolution of flare plasma parameters including temperature (T) – differential emission measure (DEM) relationship by analyzing high spectral and temporal cadence of X-ray emission in 1.6-8.0 keV energy band, recorded by SphinX (Polish) and Solar X-ray Spectrometer (SOXS; Indian) instruments, during a B8.3 flare which occurred on July 04, 2009. SphinX records X-ray emission in 1.2-15.0 keV energy band with the temporal and spectral cadence as good as 6 microsecond and 0.4 keV, respectively. On the other hand, SOXS provides X-ray observations in 4-25 keV energy band with the temporal and spectral resolution of 3 second and 0.7 keV, respectively. We derive the thermal plasma parameters during impulsive phase of the flare employing well-established Withbroe-Sylwester DEM inversion algorithm.
A. Awasthi, B. Sylwester, J. Sylwester, et. al.
Fri, 8 Apr 16
23/54
Comments: To Appear in the International Astronomical Union#320 Proceedings Series, 2015
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