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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: Pauluhn, A. et al., 1999, Applied Optics 38, 7035, also discuss the issue, deriving the pre-loss Point Spread Function (PSF) for CDS/NIS from a comparison with Sumer data. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical
  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: second order GIS 4 sensitivity with a direct cross-calibration with GIS 2 and NIS 1. ... 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: 0. and the line full-width-half-maximum FWHM (in pixels):. I =. 1. ... 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: Pike, priv. comm.) and its history, which continuously changes depending on the solar illumination. ... 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: The data indicate an isothermal distribution at log T=5.9 and are consistent with no FIP effect present. ... 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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