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31 Oct 2003: UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 11 of 41.

31 Oct 2003: The GIS is astigmatic, focusing the image of the slit along the direction of dispersion but not perpendicular to it. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 7 of 41.

31 Oct 2003: After applying VDS_DEBIAS, the units of the data are DEBIASED-ADC'. Giulio Del Zanna. ... Department of Applied Mathematics. and Theoretical Physics. 15 of 41.

31 Oct 2003: The extent in Y of the long slits (240. ¢¢. ) is therefore 143 pixels on the detector. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 12 of 41.

31 Oct 2003: Second order lines have been observed only in NIS 2. The NIS can provide monochromatic images of the solar field of view. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 6 of 41.

31 Oct 2003: 2.3 Solar rotation. The solar rotation produces an apparent movement of any feature of about 10. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 5 of 41.

31 Oct 2003: 4.6 The Radiometric Calibration in practice. There are many ways of dealing with this issue. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 30 of 41.

31 Oct 2003: UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 22 of 41.

31 Oct 2003: Use the routine gt_nis_alignment which returns the best estimate of the offset. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 19 of 41.

31 Oct 2003: For details, see the first (and still only) comprehensive in-flight calibration of all 9 CDS channels:. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 24 of 41.