7 November 1994 Ultraviolet Coronagraph Spectrometer for the Solar and Heliospheric Observatory: optical testings
Author Affiliations +
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, Silvano Fineschi, Marco Romoli, Marco Romoli, Larry D. Gardner, Larry D. Gardner, John L. Kohl, John L. Kohl, Giancarlo C. Noci, Giancarlo C. Noci, Giuseppe Tondello, 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); doi: 10.1117/12.193204; https://doi.org/10.1117/12.193204


Limits of spectral resolution in optical measurements
Proceedings of SPIE (August 21 2014)
Interference Gratings For Ultraviolet Spectroscopy
Proceedings of SPIE (February 09 1981)
Holographic Spectroscopy
Proceedings of SPIE (February 28 1974)
Polarimetry of the UV solar corona with ASCE
Proceedings of SPIE (November 24 1999)

Back to Top