The Extreme Ultraviolet Explorer Spectrometer: Performance Characteristics Based On Development Of The Collimator, Variable Line Space Gratings, Telescope And Detectors

Author(s):  
Christopher Martin ◽  
Stanley Mrowka ◽  
Stuart Bowyer ◽  
Roger F. Malina
1992 ◽  
Vol 9 ◽  
pp. 247-254 ◽  
Author(s):  
Stuart Bowyer ◽  
Patrick Jelinsky ◽  
Carol Christian ◽  
Isabel Hawkins

AbstractThe Extreme Ultraviolet Explorer mission is described. For the first six months, an all-sky survey will be carried out covering 90 to 750 Å, or essentially the entire extreme ultraviolet (EUV) bandpass. This EUV survey will be made in four bands, or colors: λλ 90-150 Å, 170-250 Å, 400-600 Å, and 550-750 Å. A portion of the sky which is free from the normally intense 304 Å geocoronal helium background will be surveyed at greater sensitivity; the wavelength coverage of this band is from 90 to 400 Å. Following the sky survey portion of the mission, spectroscopy of individual sources will be carried out. Three spectrometers employing novel variable line-space gratings will provide spectra with ~1 Å resolution over the band from 70 to 760 Å. This spectroscopy will be carried out by guest observers chosen by NASA in a manner roughly analogous to the International Ultraviolet Explorer (IUE) guest observer program.


1983 ◽  
Vol 22 (24) ◽  
pp. 3921 ◽  
Author(s):  
Michael C. Hettrick ◽  
Stuart Bowyer

1990 ◽  
Vol 123 ◽  
pp. 153-169
Author(s):  
Stuart Bowyer

AbstractThe Extreme Ultraviolet Explorer mission is described. The satellite is now scheduled to be launched in September, 1991. For the first six months, an all sky survey will be carried out covering 90 to 820 Å, or essentially the entire EUV bandpass. This EUV survey will be made in four bands, or colors, λλ90–150 Å; 170–250 Å, 400–600 Å and 550–750 Å. A portion of the sky which is free from the normally intense 304 Å geocoronal helium background will be surveyed at greater sensitivity; the wavelength coverage of this band is from 90 to 400 Å. Following the sky survey portion of the mission, spectroscopy of individual sources will be carried out. Three spectrometers employing novel variable line spaced gratings will provide spectra with ~1 Å resolution over the band from 90 to 800 Å. This spectroscopy will be carried out by guest observers chosen by NASA in a manner roughly analogous to the IUE guest observer program.


2021 ◽  
Author(s):  
Tao Ren ◽  
Keqiang Qiu ◽  
Zhengkun Liu ◽  
Yilin Hong ◽  
Xiangdong Xu ◽  
...  

2018 ◽  
Vol 45 (8) ◽  
pp. 0809001
Author(s):  
缪涛 Miao Tao ◽  
郑继红 Zheng Jihong ◽  
王康妮 Wang Kangni ◽  
刘悠嵘 Liu Yourong ◽  
黄新荣 Huang Xinrong ◽  
...  

2015 ◽  
Vol 86 (2) ◽  
pp. 023109 ◽  
Author(s):  
Qingbo Wang ◽  
Zhengkun Liu ◽  
Huoyao Chen ◽  
Yu Wang ◽  
Xiaolong Jiang ◽  
...  

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