Microflares with RHESSI and Hinode/XRT

Details Microflares with RHESSI and Hinode/XRT Microflares with RHESSI and Hinode/XRT

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..397..169h&link_type=abstract

First Results From Hinode ASP Conference Series, Vol. 397, Proceedings of the conference held 20-24 August, 2007, at Trinity Col

Astronomy and Astrophysics

Astronomy

Scientific paper

In this article we discuss the opportunities for analyzing microflares with RHESSI and Hinode/XRT. We present analysis of one microflare, using the RHESSI to obtain the thermal and non-thermal spectral parameters and compare the RHESSI images of the thermal (4-8 keV) and non-thermal (12-50 keV) emission with the Hinode/XRT images. The RHESSI non-thermal emission in this event matches spatial and temporally the initial brightest emission from XRT.

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