A hard X-ray polarimeter for gamma-ray bursts and solar flares

被引:5
作者
McConnell, ML [1 ]
Ledoux, JR [1 ]
Macri, JR [1 ]
Ryan, JM [1 ]
机构
[1] Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA
来源
X-RAY AND GAMMA-RAY TELESCOPES AND INSTRUMENTS FOR ASTRONOMY, PTS 1 AND 2 | 2003年 / 4851卷
关键词
X-ray; X-ray astronomy; gamma-ray gamma-ray astronomy; polarimetry; polarization; gamma-ray burst; solar flare;
D O I
10.1117/12.461411
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on the development of a dedicated polarimeter design that is capable of studying the linear polarization of hard X-rays (50-300 keV) from g-ray bursts and solar flares. This compact design, based on the use of a large area position-sensitive PMT (PSPMT), is referred to as GRAPE (Gamma-RAy Polarimeter Experiment). The PSPMT is used to determine the Compton interaction location within an array of small plastic scintillator elements. Some of the photons that scatter within the plastic scintillator array are subsequently absorbed by a small centrally-located array of CsI(TI) crystals that is read out by an independent multi-anode PMT. One feature of GRAPE that is especially attractive for studies of g-ray bursts is the significant off-axis response (at angles > 60). The modular nature of this design lends itself toward its accomodation on a balloon or spacecraft platform. For an array of GRAPE modules, sensitivity levels below a few percent can be achieved for both g-ray bursts and solar flares. Here we report on the latest results from the testing of a laboratory science model.
引用
收藏
页码:1382 / 1393
页数:12
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