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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/slide40-0.html
    31 Oct 2003: ob. / G(T) for each line as a function of temperature and consider the loci of these curves to constrain the shape of the emission measure distribution. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 40 of 41.
  3. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide29-0.html
    31 Oct 2003: top. The other class behaves like O V 630 A, where the intensity descreases as one goes upward from the bottom of the slit, and then levels off. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 29 of 41.
  4. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide3-0.html
    31 Oct 2003: 2.1 Slits and movements. The slits provide various fields of view (2. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 3 of 41.
  5. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide14-0.html
    31 Oct 2003: Some pre-flight information is available in Harrison et al (1995), Solar Physics, 162, 233. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 14 of 41.
  6. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide23-0.html
    31 Oct 2003: Each fitted line's parameters can be checked and modified interactively. The fit is performed with a non-linear weighted least squares fit, optimizing an initial user-supplied set of parameters ... UNIVERSITY OF CAMBRIDGE. Department of Applied
  7. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide25-0.html
    31 Oct 2003: the reflectivity of the primary mirror, the secondary mirror and the scan mirror;. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 25 of 41.
  8. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide1-0.html
    31 Oct 2003: Read CDS Software Notes. An enormous amount of information. Sign up to the CDS Software and Data Analysis Discussion List. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 1 of 41.
  9. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide8-0.html
    31 Oct 2003: Because the gain in the micro channel plates is sensitive to the intensity, the voltages applied to each detector are adjusted depending on the slit used and the solar conditions (active ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and
  10. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide16-0.html
    31 Oct 2003: Often, the number of cosmic ray hits is such that a line profile in one exposure is lost and no line intensity can be deduced. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 16 of 41.
  11. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide13-0.html
    31 Oct 2003: The Xmin Xmax numbers give the detector start and stop pixels for each data window. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 13 of 41.

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