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CDS observations of flares - slide " 5 Conclusions"
www.damtp.cam.ac.uk/user/astro/gd232/research/flares/slide9-0.html11 Jun 2003: Giulio Del Zanna. CDS observations of flares. UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. ... and Theoretical Physics. 9 of 10. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide7-0.html31 Oct 2003: Many second order lines have been observed in GIS 3 and GIS 4. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 7 of 41. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide15-0.html31 Oct 2003: Department of Applied Mathematics. and Theoretical Physics. 15 of 41. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide12-0.html31 Oct 2003: In reality, the CDS alignment is more complex, as shown in Figure 3.6.1 and described below. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 12 of 41. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide6-0.html31 Oct 2003: The spectral resolution is @ 0.35 Å for NIS 1 and @ 0.5 Å for NIS 2. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 6 of 41. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide5-0.html31 Oct 2003: the solar rotation is often a non-negligible effect in observations near sun-centre, and is further complicated by the differential rotation of the solar corona. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 5 -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide30-0.html31 Oct 2003: I recommend to analyse the 'raw' data, and apply the radiometric Calibration only at the end. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 30 of 41. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide22-0.html31 Oct 2003: See Software note #53 for details on the effect and on the broadened gaussian asymmetric profiles.. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 22 of 41. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide19-0.html31 Oct 2003: 3.7 Other geometric effects to remember. 3.7.1 Spatial offset between NIS1 and NIS2. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 19 of 41. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide24-0.html31 Oct 2003: For details, see the first (and still only) comprehensive in-flight calibration of all 9 CDS channels:. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 24 of 41.
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