Most prominent SPICE lines in the quiet Sun spectrum sorted by increasing wavelength.
|Ion||λ [nm]||log T [K]||DN/s|
|H Ly γ||97.25||4.00||39.9|
|H Ly β||102.57||4.00||171.2|
Notes. The column log T gives the line formation temperature (at the peak of the contribution function from Fig. 2). The column DN/s gives uncalibrated count rates from SPICE, obtained from fitting the line profiles of the spectrum in Fig. 1. Optionally, to obtain a rough relative calibration between the SW and LW count rates, the SW band values can be divided by a factor of 3.4 (see text for details).
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