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Date submitted: 11-Apr-1997
EFFECT OF DARK PIXELS ON TEMPERATURE AND EMISSION MEASURES Since the discovery of "dark" or radiation-damaged CCD pixels (see CCD_DARK_PIXELS in show_pix/calibration) I've worried about how seriously this problem effects temperature and emission measures derived from the images. This is a preliminary analysis to check for gross and obvious problems. The answer, at least for the two thin filters, is encouraging. The effect on temperature appears to be smaller than other sources of dispersion. The effect on emission measure is what one would expect -- the derived emission measure in the dark pixels is less than adjacent neighbors. The FR pfi data are 20 frames of an over-the-limb active region observed (first, last) = '15-JUL-96 00:11:53', '15-JUL-96 00:21:59' There were 7 Al.1 images and 13 AlMg images, all with the same ROI on the CCD. The images were dark and leak corrected with SXT_PREP and summed. The top 2 frames of the figure are difference frames prepared with the commands up2,(al-float(big_smooth(al,7,/noccd)))>(-3000)<3000 up2,(dg-float(big_smooth(dg,7,/noccd)))>(-6000)<6000. I.e., a 9-point boxcar smoothed image has been subtracted to enhance the dark pixels. The indicated sub-image is displayed in the middle pair of pictures. Here simple linearly scaled data are displayed. The dark pixels are still evident but not so dominant. The mean signals in the sub-images are 1982 and 4560 per pixels for Al.1 and AlMg respectively. Five distinct dark pixels are indicated by boxes. Temperatures and emission measures have been derived from the summed images with the command sxt_teem,2,al,3,dg,t1=total(gt_expdur(iout(iial))), $ t2=total(gt_expdur(iout(iidg))),date=iout(0),te,em. The log10(Te) and Log(EM) sub-images are displayed in the bottom panels. The mean temperature and emission measure for this sub_image are 10^6.44 and 10^44.15 respectively. The locations of the dark pixels are indicated. A cursory examination indicates no obvious correlation between dark pixels and anomalous temperatures. This would suggest that for the thin filters the proportional trapping of charge is about the same for the 2 thin filters. There IS a correlation between dark pixels and low emission measure -- as there should be. L. Acton 11-April-97