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  2. SOHO/CDS calibration page - Giulio Del Zanna

    www.damtp.cam.ac.uk/user/astro/gd232/cdscal/
    7 Feb 2003: 2000) is about 20% higher (1.64 $pm 0.12 times$ 10${-5}$), while the SERTS-97 flight has provided a value of 1.68 $pm 0.25 times$
  3. SOHO CDS Guide

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/all.htm
    31 Oct 2003: Figure 20: The proposed CDS NIS 2 sensitivity (solid line), compared with the other calibrations.. ... 2000) is about 20% higher (1.64 0.12 10. -5. ), while the SERTS-97 flight has provided a value of 1.68 0.25 10.
  4. Guide

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/exercise/cds_guide.html
    4 Nov 2003: trans=[0, 0], fov=fov,center=center,$ bottom=12,lev=[-20, -30,-40, -50, -100], lcol=green, /over, /cont plot_map, mdimap, charsize=1.4,margin=0.1, $ ... 0, 0], fov=fov,center=center,$ bottom=12,lev=[20, 30,40, 50, 100], lcol=red, /over, /cont ; NOTE: you
  5. Giulio Del Zanna's Page

    www.damtp.cam.ac.uk/user/astro/gd232/meetings.html
    11 Jun 2003: Here are some of the places I have been, attending conferences and workshops :. NATO ASI School, Bucharest, 9-20 August 1999. SOHO VIII workshop, Paris, 22-25 June 1999. ... Oslo, Norway. 17-20 June 1997. CHIANTI atomic database meeting. Arcetri, April 8
  6. CDS observations of flares - slide " 4.2  Second flare -…

    www.damtp.cam.ac.uk/user/astro/gd232/research/flares/slide8-0.html
    11 Jun 2003: However, it is interesting to note that during the previous raster, centred at 20:54:47, the same loop structure was visible (indeed had persisted for some time), while in the ... 20:49:08 21:04:49 21:08:23. 21:10:27 21:19:43 21:25:27. 20:50:34 21:03:38
  7. CDS observations of flares - slide " 3   The Cambridge AR flare …

    www.damtp.cam.ac.uk/user/astro/gd232/research/flares/slide5-0.html
    11 Jun 2003: Two types of NIS studies' were used. A diagnostic raster (1 hour and 20 minutes) that extracts many diagnostic lines;. ... a fast raster (20 minutes), but that only extracts a few lines, selected to cover a wide range of temperatures (He I 584 Å, log T
  8. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide39-0.html
    31 Oct 2003: C. 2. (T. , N. e. ). (20). Any ratios of lines of ions of close ionization stage can be used for this purpose, as long as the lines are not density-sensitive,
  9. 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 variations, around a median value of 27-28 cm. 2. (for NIS 1-2) are considerable ( 20%) over the full extent of the scan mirror positions (4.
  10. 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: 2000) is about 20% higher (1.64 0.12 10. -5. ), while the SERTS-97 flight has provided a value of 1.68 0.25 10.
  11. 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: Figure 20: The proposed CDS NIS 2 sensitivity (solid line), compared with the other calibrations..

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