The Imager for Sprites and Upper Atmospheric Lightning (ISUAL)

被引:23
作者
Frey, H. U. [1 ]
Mende, S. B. [1 ]
Harris, S. E. [1 ]
Heetderks, H. [1 ]
Takahashi, Y. [2 ,3 ]
Su, H. -T. [4 ]
Hsu, R. -R. [4 ]
Chen, A. B. [4 ]
Fukunishi, H. [3 ,5 ]
Chang, Y. -S. [6 ]
Lee, L. -C. [7 ]
机构
[1] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[2] Hokkaido Univ, Dept Earth & Planetary Sci, Sapporo, Hokkaido, Japan
[3] Tohoku Univ, Sendai, Miyagi, Japan
[4] Natl Cheng Kun Univ, Dept Phys, Tainan, Taiwan
[5] Japan Polar Res Assoc, Tokyo, Japan
[6] Natl Space Program Off, Hsinchu, Taiwan
[7] Acad Sinica, Taipei, Taiwan
关键词
TRANSIENT LUMINOUS EVENTS; GIGANTIC JETS; EMISSIONS; IONOSPHERE; IONIZATION; INSTRUMENT; SATELLITE; AIRGLOW; ENERGY; HALOS;
D O I
10.1002/2016JA022616
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Imager for Sprites and Upper Atmospheric Lightning (ISUAL) was the first specifically dedicated instrument to observe lightning-induced transient luminous events (TLE): sprites, elves, halos, and gigantic jets from space. The Imager is an intensified CCD system operating in the visible wavelength region with a filter wheel to select from six positions with filters. The Imager has a 5 degrees x 20 degrees (vertical times horizontal) field of view. The spectrophotometer (SP) is populated with six photometers with individual filters for emissions from the far ultraviolet to the near infrared. An array photometer with two channels operating in the blue and red provides altitude profiles of the emission over 16 altitude bins each. The Associated Electronics Package (AEP) controls instrument functions and interfaces with the spacecraft. ISUAL was launched 21 May 2004 into a Sun-synchronous 890 km orbit on the Formosat-2 satellite and has successfully been collecting data ever since. ISUAL is running on the nightside of the orbit and is pointed to the east of the orbit down toward the limb. The instrument runs continuously and writes data to a circular buffer. Whenever the SP detects a sudden signal increase above a preset threshold, a trigger signal is generated that commands the system to keep the data for about 400 ms starting from similar to 50 ms before the trigger. Over its lifetime of similar to 11 years the system recorded thousands of TLE and also successfully observed aurora and airglow.
引用
收藏
页码:8134 / 8145
页数:12
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