Stray light, radiometric, and spectral characterization of UVCS/SOHO: Laboratory calibration and flight performance

被引:57
|
作者
Gardner, LD
Kohl, JL
Daigneau, PS
Dennis, EF
Fineschi, S
Michels, J
Nystrom, GU
Panasyuk, A
Raymond, JC
Reisenfeld, DJ
Smith, PL
Strachan, L
Suleiman, R
Noci, G
Romoli, M
Ciaravella, A
Modigliani, A
Huber, MCE
Antonucci, E
Benna, C
Giordano, S
Tondello, G
Nicolosi, P
Naletto, G
Pernechele, C
Spadaro, D
Siegmund, OHW
Allegra, A
Carosso, P
Jhabvala, M
机构
关键词
solar physics; spectroscopy; ultraviolet; radiometry;
D O I
10.1117/12.257187
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
The Ultraviolet Coronagraph Spectrometer (UVCS) is one of the instruments on board the Solar and Heliospheric Observatory (SOHO) spacecraft, which was launched in December, 1995. The instrument is designed to make ultraviolet spectrometric measurements and visible polarimetric measurements of the extended solar corona. Prior to launch laboratory measurements were carried out to determine system level values for many of the key performance parameters. Further measurements on instrument performance have been carried out since launch. Presented are descriptions of measurement techniques and representative results.
引用
收藏
页码:2 / 24
页数:23
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