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GHRS : ウィキペディア英語版
Goddard High Resolution Spectrograph

The Goddard High Resolution Spectrograph (GHRS or HRS) was a spectrograph installed on the Hubble Space Telescope. It was replaced by the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) in 1997.〔(SM3A )〕
==GHRS facts==

*Instrument type: Ultraviolet spectrograph
*Wavelength range: 1050 to 3200 Å (105 to 320 nm)
*Resolving Power at 1200 Å (120 nm)
*
* Low - 2,000 (0.6 Å or 60 pm, or a Doppler effect of 150 km/s)
*
* Medium - 20,000 (0.06 Å or 6 pm, 15 km/s)
*
* High - 100,000 (0.012 Å or 1.2 pm, 3 km/s)
A technical description of the construction and operation of the GHRS can be found in NASA technical report CP-2244.〔, page 76. A 40 MB PDF file.〕

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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