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Giulio Del Zanna's Page
www.damtp.cam.ac.uk/user/astro/gd232/meetings.html11 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 -
CDS observations of flares - slide " 4.2 Second flare -…
www.damtp.cam.ac.uk/user/astro/gd232/research/flares/slide8-0.html11 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 -
CDS observations of flares - slide " 3 The Cambridge AR flare …
www.damtp.cam.ac.uk/user/astro/gd232/research/flares/slide5-0.html11 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 -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide28-0.html31 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. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide26-0.html31 Oct 2003: Figure 20: The proposed CDS NIS 2 sensitivity (solid line), compared with the other calibrations.. -
article
www.damtp.cam.ac.uk/user/astro/gd232/research/flares/all.htm6 Apr 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 -
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 $pm 0.25 times$ -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide27-0.html31 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. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide20-0.html31 Oct 2003: UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 20 of 41. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide39-0.html31 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, -
Guide
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/exercise/cds_guide.html4 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 -
SOHO CDS Guide
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/all.htm31 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.
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