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  1. Results that match 1 of 2 words

  2. Thursday Seminars on Theoretical Geophysics

    www.itg.cam.ac.uk/seminars/thu_2.05/mich_2003.html
    13 Oct 2003: 20 November. Gordon Woo. (Risk Management Solutions). Catastrophe risk. 27 November.
  3. Thursday Seminars on Theoretical Geophysics

    www.itg.cam.ac.uk/seminars/thu_2.05/lent_2003.html
    29 Jan 2003: 20 February. Andy Woods. (BPI). Models of flows in oil reservoirs.
  4. 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,
  5. 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.
  6. 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.
  7. 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..
  8. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide20-0.html
    31 Oct 2003: UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 20 of 41.
  9. 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
  10. 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.
  11. 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

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