Slajd 1

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Envisaging SphinX forward modeling of X-ray
spectra M. Siarkowski Space Research Centre
PAS, Solar Physics Division, Wroclaw, POLAND
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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
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SF IDL routines for calculating atomic
scattering factors (Lawrence Berkeley NL)
http//physics.nist.gov/PhysRefData/XrayMassCoef/
thickness error 10
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Temperature and Emission Measure vs. Flare Class
Bak-Steslicka, 2006
Garcia, 1994
Bak-Steslicka, 2006
Feldman, 1995
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Temperature and Emission Measure vs. Flare Class
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Te MK
3
Log EM
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Te EM CHIANTI v5.2
spectra
46.5
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Spinx spectra
D2
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Spinx spectra
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Spinx spectra
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Spinx spectra
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Spinx spectra
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Spinx spectra
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Spinx spectra
D2
Fe
Mg Al Si
S
Ar
Si S
Ca
Fe
Ni
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end