File:Mem njit event3 dist.jpg.jpg

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Energy dependence of the distance, D, between the peak in coronal flux in the 20-22 keV image and the peak at other energies. The solid lines show linear fits to the data points from 10 to 20 keV and 20 to 30 keV, and the indicated values of DeltaD are the changes in position in arcsec over the two energy ranges.

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current21:29, 21 September 2018Thumbnail for version as of 21:29, 21 September 20181,052×1,052 (156 KB)Bdennis (Talk | contribs) (Energy dependence of the distance, D, between the peak in coronal flux in the 20-22 keV image and the peak at other energies. The solid lines show linear fits to the data points from 10 to 20 keV and 20 to 30 keV, and the indicated values of DeltaD are th)

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