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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: 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: This correction is accurate (to a few percent) only for the bright and un-blended lines.. ... 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: Figure 4: [from MSSL user guide] A GIS 1 spectrum output from ghost_plot_one, (top-top) theoretical quiet sun spectrum, (top-middle) left shifted spectrum, (top-bottom) right shifted spectrum. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics

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