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The Solar Wind Charge-eXchange Contribution to the Local Soft X-ray Background. Model to Data Comparison in the 0.1–1.0 keV Band

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Figure

Fig. 1 SWCX model spectra in Line Units (photons cm −2 s −1 sr −1 ) for the 3/4 keV band
Fig. 2 Calculated full sky maps in ecliptic coor- coor-dinates of the 0.65 keV O VIII line for solar max-imum (upper panel) and solar minmax-imum (lower panel) conditions
Fig. 3 Top: O VII and O VIII line simulated lightcurves (in LU) for the MBM12 ON and OFF obser-vations with Suzaku during the period 03-08/02/2006
Table 1 Comparison of shadowing observation foreground data to SWCX model for O VII and O VIII line intensities
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