Paper
7 November 1994 Ultraviolet Coronagraph Spectrometer for the Solar and Heliospheric Observatory: optical testings
Silvano Fineschi, Marco Romoli, Larry D. Gardner, John L. Kohl, Giancarlo C. Noci, Giuseppe Tondello
Author Affiliations +
Abstract
The Ultraviolet Coronagraph Spectrometer (UVCS) of the Solar and Heliospheric (SOHO) mission has been developed for spectroscopic and polarimetric determinations of temperatures, densities and flow velocities in the extended solar corona. The instrument consists of two ultraviolet (UV) spectrometers and a visible light (VL) polarimeter. The grating of the UV channel optimized for the HI Lyman (alpha) (Ly-(alpha) ) line ((lambda) 1236 angstrom) and that for the OVI doublet ((lambda) (lambda) 1032/1037 angstrom) have been characterized.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Silvano Fineschi, Marco Romoli, Larry D. Gardner, John L. Kohl, Giancarlo C. Noci, and Giuseppe Tondello "Ultraviolet Coronagraph Spectrometer for the Solar and Heliospheric Observatory: optical testings", Proc. SPIE 2283, X-Ray and Ultraviolet Spectroscopy and Polarimetry, (7 November 1994); https://doi.org/10.1117/12.193204
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Cited by 2 scholarly publications.
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KEYWORDS
Holography

Diffraction gratings

Diffraction

Polarization

Stray light

Coronagraphy

Solar processes

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