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  2. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide21-0.html
    31 Oct 2003: S. V. H. Haugan discusses in Anomalous Line Shifts from Local Intensity Gradients on the SOHO/CDS NIS Detector (Solar Physics 185, 275, 1999) the NIS PSF. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 21 of 41.
  3. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide28-0.html
    31 Oct 2003: The narrow solid line shows the behavior derived from He I 584 A, and the dashed line shows the behavior derived from O V 630 A, both normalized to the theoretical ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics.
  4. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide32-0.html
    31 Oct 2003: These types of spectra have been mainly used for the first order internal and cross-detector calibration.. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 32 of 41.
  5. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide31-0.html
    31 Oct 2003: is the number of pixels being summed over and R is the readout noise per pixel. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 31 of 41.
  6. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide26-0.html
    31 Oct 2003: Note that neither the ground calibration measurements nor the theoretical predictions of the sensitivities are in accordance with both the direct in-flight results of Brekke et al. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and
  7. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide27-0.html
    31 Oct 2003: The bottom right plot shows the ratio of the theoretical vs. ... Department of Applied Mathematics. and Theoretical Physics. 27 of 41.
  8. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide20-0.html
    31 Oct 2003: IDL> qwavecal. The slant of the two channels, and the tilt of the lines complicates the wavelength determination. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 20 of 41.
  9. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide41-0.html
    31 Oct 2003: dT. dT. (21). Many authors (e.g. Pottasch 1963; Jordan and Wilson 1971) approximate the above expression by removing an averaged value of C(T) from the integral:. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics.
  10. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide17-0.html
    31 Oct 2003: The image on the right shows the same data after the standard corrections have been applied.. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 17 of 41.
  11. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide9-0.html
    31 Oct 2003: Once the applied LUTs are known, it is therefore possible to deduce which regions of the spectrum are unlikely to be affected by them, and to predict where ghosts might appear. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and

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