Correlation between decimetric radio emission and hard X-rays in solar flares

B. P. Dąbrowski; A. O. Benz

doi:10.1051/0004-6361/200811108

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Volume 504 / No 2 (September III 2009)

A&A, 504 2 (2009) 565-573

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Table 2:

Analyzed groups of decimetric spikes.
Date	Start time	End time	pos^a	$E\_l$ ^b	$\nu$ ^c	cc $\_G$ ^d	$\Delta t\_G$ ^e	cc $\_{max}$ ^f	$\Delta t\_{max}$ ^g	$\phi\_{GOES}$ ^h	$\phi\_{\it RHESSI}$ ⁱ
[dd.mm.yy]	[hh:mm:ss]	[hh:mm:ss]	['']	[keV]	[MHz]		[s]		[s]	[W m^-2]	[ct/s/subcoll]
14.08.04	12:03:53	12:05:25	590	20	1865-2950	0.69	1.32	0.77	-1.00	$4.78\times10^{-6}$	44.4
19.01.04	12:33:46	12:34:21	193	25	685-1300	0.70	0.65	0.74	0.73	$4.70\times10^{-6}$	224.1
10.06.03	11:08:27	11:09:19	683	19	650-1570	0.81	-2.40	0.82	-2.70	$2.19\times10^{-5}$	122.5
09.01.03	13:20:31	13:21:14	850	25	515-904	0.63	0.85	0.65	1.15	$1.51\times10^{-6}$	13.6
20.12.02	14:19:04	14:19:55	623	15	983-1845	0.90	-1.71	0.95	-1.70	$1.98\times10^{-6}$	33.8
20.09.02	12:37:16	12:40:52	444	10	632-1540	0.65	2.06	0.68	1.61	$1.02\times10^{-6}$	25.5
29.07.02	11:02:14	11:03:46	371	18	632-1415	0.64	-10.64	0.66	-12.56	$3.59\times10^{-5}$	270.8
29.07.02	11:05:53	11:07:23	371	18	623-1090	0.75	-11.95	0.78	-8.83	$3.23\times10^{-5}$	213.6
15.07.02	11:44:24	11:44:50	229	25	542-721	0.88	-0.57	0.88	0.07	$3.82\times10^{-6}$	242.9
11.06.03*	16:27:29	16:29:56	849	25	381-784	0.32	-4.55	0.32	-0.49	$3.60\times10^{-5}$	154.7
15.07.02*	11:44:25	11:45:05	229	25	721-1210	0.76	-0.58	0.78	0.10	$3.99\times10^{-6}$	190.8

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