Fine-pitch CdTe detector for hard X-ray imaging and spectroscopy of the Sun with the FOXSI rocket experiment

被引:12
作者
Ishikawa, Shin-nosuke [1 ]
Katsuragawa, Miho [1 ,2 ]
Watanabe, Shin [1 ,2 ]
Uchida, Yuusuke [1 ,2 ]
Takeda, Shin'ichiro [3 ]
Takahashi, Tadayuki [1 ,2 ]
Saito, Shinya [4 ]
Glesener, Lindsay [5 ]
Buitrago-Casas, Juan Camilo [6 ]
Krucker, Sam [6 ,7 ]
Christe, Steven [8 ]
机构
[1] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa, Japan
[2] Univ Tokyo, Grad Sch Sci, Tokyo, Japan
[3] Okinawa Inst Sci & Technol Grad Univ, Adv Med Instrumentat Unit, Onna, Okinawa, Japan
[4] Rikkyo Univ, Dept Phys, Bunkyo Ku, Tokyo, Japan
[5] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
[6] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[7] Univ Appl Sci Northwestern Switzerland, Inst Technol 4D, Sch Engn, Windisch, Switzerland
[8] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
基金
日本学术振兴会;
关键词
Sun; X-ray; solar corona; semiconductor detector; imaging spectroscopy; SOLAR-A MISSION; DIODE DETECTORS; NUSTAR; FLARES; REGION; RHESSI; IMAGER; LOOP;
D O I
10.1002/2016JA022631
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have developed a fine-pitch hard X-ray (HXR) detector using a cadmium telluride (CdTe) semiconductor for imaging and spectroscopy for the second launch of the Focusing Optics Solar X-ray Imager (FOXSI). FOXSI is a rocket experiment to perform high sensitivity HXR observations from 4 to 15keV using the new technique of HXR focusing optics. The focal plane detector requires <100m position resolution (to take advantage of the angular resolution of the optics) and approximate to 1keV energy resolution (full width at half maximum (FWHM)) for spectroscopy down to 4keV, with moderate cooling (>-30 degrees C). Double-sided silicon strip detectors were used for the first FOXSI flight in 2012 to meet these criteria. To improve the detectors' efficiency (66% at 15keV for the silicon detectors) and position resolution of 75m for the second launch, we fabricated double-sided CdTe strip detectors with a position resolution of 60m and almost 100% efficiency for the FOXSI energy range. The sensitive area is 7.67mmx7.67mm, corresponding to the field of view of 791x791. An energy resolution of 1keV (FWHM) and low-energy threshold of approximate to 4keV were achieved in laboratory calibrations. The second launch of FOXSI was performed on 11 December 2014, and images from the Sun were successfully obtained with the CdTe detector. Therefore, we successfully demonstrated the detector concept and the usefulness of this technique for future HXR observations of the Sun.
引用
收藏
页码:6009 / 6016
页数:8
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