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CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide21-0.html31 Oct 2003: Pauluhn, A. et al., 1999, Applied Optics 38, 7035, also discuss the issue, deriving the pre-loss Point Spread Function (PSF) for CDS/NIS from a comparison with Sumer data. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical -
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 CDS routine GET_EFF_AREA provides the pre-flight values of A. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 28 of 41. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide32-0.html31 Oct 2003: Figure 31: The NIS 2 spectrum of an on-disc quiet sun observation. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 32 of 41. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide31-0.html31 Oct 2003: 1). In the case of n. avg. spectra averaged, we have to divide s. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 31 of 41. -
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: The only direct in-flight absolute calibration study is that of Brekke et al. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 26 of 41. -
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; 1.32 0.11 10. -5. ). The measurement of Brekke et al. ... Department of Applied Mathematics. and Theoretical Physics. 27 of 41. -
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: The solid line is a polynomial fit to the average of the two lines.. ... 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/slide41-0.html31 Oct 2003: 5. K. -1. ]. (24). such that for each line of observed intensity I. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide17-0.html31 Oct 2003: The image on the right shows the same data after the standard corrections have been applied.. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 17 of 41. -
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 - slide…
www.damtp.cam.ac.uk/user/astro/gd232/research/medoc_03/slide9-0.html31 Oct 2003: Now, once a set of LUTs is applied to the data on-board, i.e. ... UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics. and Theoretical Physics. 9 of 41.
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