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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/slide11-0.html
    31 Oct 2003: delete_qlds,qlds ; delvarx, QLDS WOULD NOT WORK! ;--------------------------------. Once the data have been loaded, the QuickLook package can be used to inspect (and analyse) them:. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and
  3. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide7-0.html
    31 Oct 2003: Many second order lines have been observed in GIS 3 and GIS 4. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 7 of 41.
  4. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide15-0.html
    31 Oct 2003: Department of Applied Mathematics. and Theoretical Physics. 15 of 41.
  5. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide12-0.html
    31 Oct 2003: In reality, the CDS alignment is more complex, as shown in Figure 3.6.1 and described below. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 12 of 41.
  6. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide6-0.html
    31 Oct 2003: The spectral resolution is @ 0.35 Å  for NIS 1 and @ 0.5 Å  for NIS 2. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 6 of 41.
  7. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide5-0.html
    31 Oct 2003: the solar rotation is often a non-negligible effect in observations near sun-centre, and is further complicated by the differential rotation of the solar corona. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 5
  8. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide30-0.html
    31 Oct 2003: I recommend to analyse the 'raw' data, and apply the radiometric Calibration only at the end. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 30 of 41.
  9. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide22-0.html
    31 Oct 2003: See Software note #53 for details on the effect and on the broadened gaussian asymmetric profiles.. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 22 of 41.
  10. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide19-0.html
    31 Oct 2003: 3.7 Other geometric effects to remember. 3.7.1 Spatial offset between NIS1 and NIS2. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 19 of 41.
  11. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide24-0.html
    31 Oct 2003: For details, see the first (and still only) comprehensive in-flight calibration of all 9 CDS channels:. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 24 of 41.

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