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Table 2.

Total radiative fluxes of the chromosphere from H continua (Balmer to Pfundt) in different flare models.

Flare (109 erg cm−2) (%)
model detailed this work this work
Models for fitting

f10E05d3 9.00 8.36 −7.09
f10E10d3 11.05 8.55 −22.62
f10E15d3 14.59 10.82 −25.88
f10E20d3 17.81 12.91 −27.55
f10E25d3 21.48 15.37 −28.44
f10E05d4 5.40 6.33 17.27
f10E10d4 7.42 7.03 −5.22
f10E15d4 8.97 7.76 −13.45
f10E20d4 12.24 10.08 −17.66
f10E25d4 16.17 12.92 −20.07
f10E05d5 3.76 4.81 27.80
f10E10d5 6.04 6.44 6.48
f10E15d5 6.08 5.84 −3.88
f10E20d5 8.98 7.93 −11.70
f10E25d5 12.56 10.62 −15.57
f10E05d6 2.93 3.93 34.19
f10E10d6 5.40 6.09 12.83
f10E15d6 4.53 4.60 1.62
f10E20d6 7.10 6.62 −6.87
f10E25d6 10.44 9.11 −12.82
f10E05d7 2.48 3.45 39.01
f10E10d7 5.01 5.83 16.38
f10E15d7 3.78 3.85 2.11
f10E20d7 5.98 5.77 −3.48
f10E25d7 9.10 8.11 −10.84

Models for test

f11E15d3 147.04 122.94 −16.39
f11E20d4 109.77 110.19 0.38
f11E25d5 87.93 76.61 −12.87

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