THE MIDDLE ATMOSPHERE HIGH-RESOLUTION SPECTROGRAPH INVESTIGATION

被引：0
|
作者：
SEELEY, TD
CONWAY, RR
CARRUTHERS, GR
机构：
来源：
INSTITUTE OF PHYSICS CONFERENCE SERIES | 1992年 / 121期
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D O I：
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中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The Middle Atmosphere High Resolution Spectrograph Investigation (MAHRSI) will obtain very high resolution spectra in the middle-UV wavelength range (198-310 nm with 0.01 nm resolution), in the mesosphere from near-Earth orbit. Its primary objective is to measure hydroxyl (OH) and nitric oxide (NO) in this region of the atmosphere. MAHRSI uses a Czerny-Turner spectrograph with an image-intensified CCD (ICCD) detector. The combination of a magnetically-focused image tube with Cs2Te photocathode and a large-format CCD provides high resolution, broad instantaneous spectral coverage, and a very wide dynamic range.
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页码：41 / 48
页数：8
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