1. Envisaging SphinX: forward modeling of X-ray spectra M. Siarkowski Space Research Centre PAS, Solar Physics Division, Wroclaw, POLAND

2. XR-100CR Efficiency Curves Figure 2 (linear). Shows the intrinsic full energy detection efficiency for the XR-100CR detectors. This efficiency corresponds to the probability that an X-ray will enter the front of the detector and deposit all of its energy inside the detector via the photoelectric effect

4. http://physics.nist.gov/PhysRefData/XrayMassCoef/ SF: IDL routines for calculating atomic scattering factors (Lawrence Berkeley NL) thickness error ± 10 %

5. Feldman, 1995 Garcia, 1994 Bąk-Stęślicka, 2006 Temperature and Emission Measure vs. Flare Class

6. 3 20 46.5 50 Log EM Te [MK] Temperature and Emission Measure vs. Flare Class e EM T e EM CHIANTI v5.2 spectra

8. Spinx spectra D2

9. Spinx spectra

14. D2 Fe Mg Al Si S Ar Ca Fe Ni S

15. end