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Table 1.

Observed and predicted radiances for microflare loop-top region, with raster start at 14:19 UT.

λobs Iobs Tmax Teff R Ion λexp r
(Å) (log) (log) (Å)
192.93 81 5.42 5.56 0.64 O V 192.904 0.84
248.50 70 5.42 5.67 1.02 O V 248.461 0.78
Al VIII 248.459 0.21
184.53 789 6.05 6.12 1.15 Fe X 184.537 0.93
192.80 415 5.42 6.16 0.99 Fe XI 192.813 0.92
192.38 905 6.20 6.23 1.20 Fe XII 192.394 0.97
264.79 2910 6.29 6.37 0.89 Fe XIV 264.789 0.94
274.21 2410 6.29 6.38 1.03 Fe XIV 274.204 0.95
192.02 130 7.19 6.50 1.03 Fe XXIV 192.028 0.14
Fe XI 192.021 0.76
284.16 30800 6.34 6.52 0.97 Fe XV 284.163 0.99
195.25 96.4 6.44 6.53 1.15 Ni XVI 195.271 0.91
262.99 4200 6.43 6.62 0.93 Fe XVI 262.976 0.99
254.90 463 6.74 6.68 1.01 Fe XVII 254.885 0.99
192.84 1720 6.76 6.71 0.94 Ca XVII 192.853 1.0
263.76 3 (ul) 7.16 7.11 1.04 Fe XXIII 263.766 0.96

Notes. Each line lists the observed wavelengths λobs (Å), the measured radiances Iobs (ergs cm−2 s−1 sr−1), the maximum and effective temperature (log values, in K; see text) Tmax and Teff, the ratio R between the predicted and observed values, the main contributing ion and CHIANTI wavelength λexp (Å), and the fractional contribution r (only contributions greater than 10% are shown) to the blend. (ul) indicates an upper limit.

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