The Imaging Ultraviolet Spectrograph (IUVS) for the MAVEN Mission

被引：164
|
作者：
McClintock, William E. [1 ]
Schneider, Nicholas M. [1 ]
Holsclaw, Gregory M. [1 ]
Clarke, John T. [2 ]
Hoskins, Alan C. [1 ]
Stewart, Ian [1 ]
Montmessin, Franck [3 ]
Yelle, Roger V. [4 ]
Deighan, Justin [1 ]
机构：
[1] Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80303 USA
[2] Boston Univ, Dept Astron, Boston, MA 02215 USA
[3] CNRS, LATMOS, Guyancourt, France
[4] Univ Arizona, Dept Planetary Sci, Lunar & Planetary Lab, Tucson, AZ 85726 USA
来源：
SPACE SCIENCE REVIEWS | 2015年 / 195卷 / 1-4期
基金：
美国国家航空航天局;
关键词：
Atmosphere; Exosphere; Mars; MAVEN; Spectrograph; Ultraviolet; SPECTROMETER EXPERIMENT; UPPER-ATMOSPHERE; FAR-ULTRAVIOLET; DIFFRACTION GRATINGS; MARS; HYDROGEN; SPECTROSCOPY; CALIBRATION; TELESCOPE; STABILITY;
D O I：
10.1007/s11214-014-0098-7
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Imaging Ultraviolet Spectrograph (IUVS) is one of nine science instruments aboard the Mars Atmosphere and Volatile and EvolutioN (MAVEN) spacecraft. MAVEN, launched in November 18, 2013 and arriving at Mars in September 2014, is designed to explore the planet's upper atmosphere and ionosphere and examine their interaction with the solar wind and solar ultraviolet radiation. IUVS is one of the most powerful spectrographs sent to another planet, with several key capabilities: (1) separate Far-UV & Mid-UV channels for stray light control, (2) a high resolution echelle mode to resolve deuterium and hydrogen emission, (3) internal instrument pointing and scanning capabilities to allow complete mapping and nearly-continuous operation, and (4) optimization for airglow studies.
引用
收藏
页码：75 / 124
页数：50
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