Table 1: Upper level u, wavelength $\lambda_0 [\AA]$, spectral line radiance $E^{\rm obs}_{\rm ul}[{\rm mW}/({\rm m}^2~{\rm s}~{\rm sr})]$, spectral radiance at line center $L_{u1}(\lambda _0) [{\rm mW}/({\rm m}^2~{\rm s}~{\rm sr}~\AA)]$, and corresponding brightness temperature $T_{\rm b}$ [K] for Lyman lines of the two prominence regions given in Fig. 1 as rhombs and squares.

u		 $\lambda_0$   brightest     faintest  
    $E^{\rm obs}_{u1}$ $L_{u1}(\lambda _0)$ $T_{\rm b}$ $E^{\rm obs}_{u1}$ $L_{u1}(\lambda _0)$ $T_{\rm b}$
5 949.8 69.1 0.057 4899 25.9 0.022 4752
6 937.8 36.8 0.077 4999 14.1 0.031 4855
7 930.8 23.3 0.056 4979 9.0 0.023 4841
8 926.2 18.0 0.051 4985 6.9 0.020 4840
9 923.2 15.7 0.045 4979 6.0 0.016 4820
10 921.0 12.1 0.039 4966 4.2 0.014 4809
11 919.4 12.4 0.040 4977 4.2 0.015 4827
12 918.1 13.3 0.042 4991 3.6 0.012 4799
13 917.2 10.2 0.037 4975 4.2 0.016 4864
14 916.4 11.9 0.045 5009 2.9 0.011 4794
16 915.3 11.0 0.037 4983 3.6 0.014 4835
17 914.9 10.4 0.037 4985 7.9 0.012 4814
18 914.6 10.3 0.034 4973 2.6 0.012 4815
19 914.3 13.1 0.033 4970 4.2 0.011 4803


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