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1 - 9 of 9 search results for news |u:www.damtp.cam.ac.uk

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  2. Giulio Del Zanna -- Atomic data

    www.damtp.cam.ac.uk/user/astro/gd232/research/atom.html
    2 Jul 2003: I've produced new compilations of atomic data, written two CHIANTI user guides, and designed the WWW pages:.

  3. Giulio Del Zanna -- Solar Active regions

    www.damtp.cam.ac.uk/user/astro/gd232/research/ar.html
    15 Jun 2003: G. Del Zanna and H.E. Mason, A&A, 2003, in press. A new view of active regions is presented.

  4. CDS observations of flares - slide " 4  The big flare of 2001…

    www.damtp.cam.ac.uk/user/astro/gd232/research/flares/slide6-0.html
    11 Jun 2003: 9 hours after the flare. The activity, however, was still at high levels with continuing new small flares occurring.

  5. Giulio Del Zanna -- High-resolution X-ray spectroscopy

    www.damtp.cam.ac.uk/user/astro/gd232/research/x-ray.html
    11 Jun 2003: New results, significantly different from those of the prvious literature are found.

  6. CDS observations of flares - slide " 4.1   First flare -…

    www.damtp.cam.ac.uk/user/astro/gd232/research/flares/slide7-0.html
    11 Jun 2003: Figure 7: CDS monochromatic images of one diagnostic raster - 2001 Apr 10 18:03-19:27 UT - A new Fe XIX flare emission appeared in the NW corner, associated with a

  7. Giulio Del Zanna -- Spectroscopic diagnostics and applications

    www.damtp.cam.ac.uk/user/astro/gd232/research/diagnostics.html
    11 Jun 2003: New results, significantly different from those of the prvious literature are found.

  8. Giulio Del Zanna PhD page

    www.damtp.cam.ac.uk/user/astro/gd232/research/thesis/
    11 Jun 2003: Abstract. New Extreme Ultra-Violet (EUV) observations of the solar corona, obtained by the Coronal Diagnostic Spectrometer (CDS) instrument on board the NASA/ESA Solar and Heliospheric Observatory (SOHO) are presented. ... resulting in several new line

  9. Estimating AR electron densities at coronal temperatures with CDS…

    www.damtp.cam.ac.uk/user/astro/gd232/cds/densities/densities.html
    5 May 2003: Only recently, new calculations (Storey et al., 1999) have shed light on the Fe XIV problem.

  10. article

    www.damtp.cam.ac.uk/user/astro/gd232/research/flares/all.htm
    6 Apr 2003: 9 hours after the flare. The activity, however, was still at high levels with continuing new small flares occurring. ... Figure 7: CDS monochromatic images of one diagnostic raster - 2001 Apr 10 18:03-19:27 UT - A new Fe XIX flare emission appeared in

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