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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: Images of the Sun are obtained using a pinhole slit and combining movements of the slit and of the scan mirror. ... 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: After applying VDS_DEBIAS, the units of the data are DEBIASED-ADC'. Giulio Del Zanna. ... 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: The VDS detector is mainly composed of a microchannel plate and a 1024x1024 pixels charge coupled device (CCD), composed of four square sections. ... 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: This is accomplished with the rastering of a region, moving a mirror and producing contiguous images of one of the long slits. ... 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: 4.6 The Radiometric Calibration in practice. There are many ways of dealing with this issue. ... 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: 3.7.2 Spatial offset between NIS anf GIS. There is also an offset between the imaging of NIS and GIS. ... 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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