Search

Search Funnelback University

Search powered by Funnelback
31 - 40 of 53 search results for `Department of Applied Mathematics` |u:www.damtp.cam.ac.uk
  1. Fully-matching results

  2. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide40-0.html
    31 Oct 2003: ob. / G(T. i. ) represents an upper limit to the value of the line emission measure EM. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 40 of 41.
  3. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide29-0.html
    31 Oct 2003: Other lines, such as He I 584 A, can be modelled as a linear combination of these two behaviors.. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 29 of 41.
  4. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide3-0.html
    31 Oct 2003: 2.1 Slits and movements. The slits provide various fields of view (2. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 3 of 41.
  5. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide14-0.html
    31 Oct 2003: Routines to calculate the amount of scattered light and an explanation of how to apply them are available at:. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 14 of 41.
  6. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide23-0.html
    31 Oct 2003: The fitting is done passing a series of initial parameters that define each line to be fitted. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 23 of 41.
  7. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide25-0.html
    31 Oct 2003: the reflectivity of the primary mirror, the secondary mirror and the scan mirror;. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 25 of 41.
  8. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide1-0.html
    31 Oct 2003: Read CDS Software Notes. An enormous amount of information. Sign up to the CDS Software and Data Analysis Discussion List. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 1 of 41.
  9. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide8-0.html
    31 Oct 2003: Because the gain in the micro channel plates is sensitive to the intensity, the voltages applied to each detector are adjusted depending on the slit used and the solar conditions (active ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and
  10. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide16-0.html
    31 Oct 2003: An effect that strongly constrains the observations is the presence of cosmic ray hits. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 16 of 41.
  11. CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…

    www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide13-0.html
    31 Oct 2003: The wavelengths are calculated using an average pixel-wavelength conversion applicable to the date of observation. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 13 of 41.

Refine your results

Search history

Recently clicked results

Recently clicked results

Your click history is empty.

Recent searches

Recent searches

Your search history is empty.