Optical design of the coronal diagnostic spectrometer (an instrument on the Solar and Heliospheric Observatory)

Details Optical design of the coronal diagnostic spectrometer (an instrument on the Solar and Heliospheric Observatory) Optical design of the coronal diagnostic spectrometer (an instrument on the Solar and Heliospheric Observatory)

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997opten..36.2311l&link_type=abstract

Optical Engineering 36(08), 2311-2319, Brian J. Thompson; Ed.

Computer Science

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3

Scientific paper

The coronal diagnostic spectrometer (CDS) is one of 12 instruments that form the payload of the joint European Space Agency/National Aeronautics and Space Agency Solar and Heliospheric Observatory, launched in 1995. The CDS was designed and constructed by an international consortium led by the Rutherford Appleton Laboratory, United Kingdom. It is a high resolution, extreme UV telescope and spectrometer for making observations of the high temperature outer regions of the sun. The optical system is described and the theoretical performance of the design is discussed.

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