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The CDS instrument (Figure 1) consists of a Wolter-Schwartzschild type II grazing incidence telescope, a scan mirror, a set of different slits, and two spectrometers that do not observe simultaneously, the normal incidence spectrometer (NIS) and the grazing incidence spectrometer (GIS).
CDS data analysis + spectroscopy using CHIANTI - MEDOC 2003 |
UNIVERSITY OF CAMBRIDGE Department of Applied Mathematics and Theoretical Physics |
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