Diagnostics of non-thermal distributions in solar flare spectra observed by RESIK and RHESSI

Free Access

Issue		A&A Volume 533, September 2011


Article Number		A81
Number of page(s)		16
Section		The Sun
DOI		https://doi.org/10.1051/0004-6361/201116741
Published online		30 August 2011

Online material

Appendix A: Complementary figures and tables

Table A.1

Time-weighted RESIK spectra for the C5.8 flare on February 22, 2003 and the determined ranges of the parameters n and log τ.

Table A.2

Results from RHESSI analysis of the 2003 February 22 flare.

Table A.3

Time-weighted RESIK spectra for the M4.9 flare on January 7, 2003. Notation is the same as in Table A.1.

Table A.4

Results from RHESSI analysis of the 2003 January 7 flare. Notation is the same as in Table A.2.

Table A.5

Time-weighted RESIK spectra for the M4.0 flare on October 4, 2002. Notation is the same as in Table A.1.

Table A.6

Results from RHESSI analysis of the 2002 October 4 flare. Notation is the same as in Table A.2.

Table A.7

Details of the RHESSI spectrum fitting (2003 February 22, 09:28:12–09:28:20 UT) and comparison with the corresponding RESIK results (09:27:43–09:28:31 UT).

Table A.8

Details of the RHESSI spectrum fitting (2003 January 7, 23:28:32–23:28:52 UT) and comparison with the corresponding RESIK results (23:28:25–23:29:17 UT). Notation is the same as in Table A.7.

	Fig. A.1 RHESSI fits (from 6 keV) of the single power law (thick-target model) and the thermal component together with residuals: the 2003 February 22 flare (left) and the 2003 January 7 flare (right).
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	Fig. A.2 Widened RHESSI fits (from 4 keV). Notation is the same as in Fig. A.1.
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© ESO, 2011

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