Differential emission measure analysis of active region cores and quiet Sun for the non-Maxwellian κ-distributions

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Table 4

List of spectral lines from Landi & Young (2010) used in the reconstruction of DEM by W-S method and RIM. The I^obs, R_Maxw, and R_{κ = 2} are shown.

Ion	λ [Å]	I ^obs	W-S method		RIM
Ion	λ [Å]	I ^obs	R _Maxw	R _{κ = 2}	R _Maxw	R _{κ = 2}


Fe viii	185.21	14.6	1.20	1.45	0.80	0.98
Fe viii	186.60	11.0	1.01	1.28	0.68	0.86
Fe viii	194.66	3.90	1.27	1.46	0.86	0.99
Fe x	174.53	244.	1.07	0.96	0.62	0.63
Fe x	175.26	18.0	1.54	1.36	0.88	0.87
Fe x	177.24	153.	0.94	0.85	0.55	0.56
Fe xi	178.06	9.10	1.04	0.94	0.68	0.65
Fe xi	180.40	208.	0.99	0.92	0.65	0.65
Fe xi	180.59	7.50	1.18	1.14	0.77	0.79
Fe xi	181.13	10.1	1.23	1.19	0.80	0.83
Fe xi	182.17	35.6	0.96	0.87	0.62	0.61
Fe xi	201.73	5.70	1.18	1.11	0.76	0.77
Fe xii	186.89	24.9	0.93	0.78	0.71	0.59
Fe xii	192.39	46.6	0.84	0.81	0.66	0.63
Fe xii	193.51	85.0	0.96	0.93	0.75	0.73
Fe xii	195.12	134.	0.90	0.87	0.71	0.68
Fe xii	196.12	8.50	0.87	0.74	0.66	0.56
Fe xii	249.39	5.70	0.64	0.70	0.49	0.53
Fe xiii	202.04	87.3	0.46	0.54	0.47	0.49
Fe xiii	203.16	3.20	1.02	1.10	0.98	0.93
Fe xiii	203.83	20.3	0.99	1.02	0.94	0.86
Fe xiii	204.94	5.80	0.71	0.79	0.70	0.70
Fe xiv	270.52	7.50	0.68	0.96	0.85	0.93
Fe xiv	274.20	19.4	0.56	0.81	0.71	0.79
Fe xv	284.16	26.8	0.73	1.22	1.09	1.19

	χ		0.24	0.23	0.30	0.30

Notes. The Hinode/EIS intensities have units erg cm^-2 s^-1 sr^-1.

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