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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: Bill Thompson analysed NISAT_S, NIMCP, and SYNOP_F data and came up with the following conclusions. ... 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: Line profiles can have any general shape, and the background' is normally fitted with a polynomial. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 23 of 41.
  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 IDL procedures headers. Get involved! Be open-minded and do not take any results for granted. ... 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: 3.4 Cosmic ray removal. See CDS software Note 46: Missing Pixels and Cosmic Rays for details. ... 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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