The Spectrometer Telescope for Imaging X-rays (STIX) on board the Solar Orbiter mission

被引：22

作者：

Benz, A. O. ^{[1
]}

Krucker, S. ^{[1
]}

Hurford, G. J. ^{[1
]}

Arnold, N. G. ^{[1
]}

Orleanski, P. ^{[1
]}

Groebelbauer, H. -P. ^{[1
]}

Kobler, S. ^{[1
]}

Iseli, L. ^{[1
]}

Wiehl, H. J. ^{[1
]}

Csillaghy, A. ^{[1
]}

Etesi, L. ^{[1
]}

Hochmuth, N. ^{[1
]}

Battaglia, M. ^{[1
]}

Bednarzik, M.

Resanovic, R.

Grimm, O.

Viertel, G.

Commichau, V.

Meuris, A.

Limousin, O.

Brun, S.

Vilmer, N.

Skup, K. R.

Graczyk, R.

Stolarski, M.

Michalska, M.

Nowosielski, W.

Cichocki, A.

Mosdorf, M.

Seweryn, K.

Przepiorka, A.

Sylwester, J.

Kowalinski, M.

Mrozek, T.

Podgorski, P.

Mann, G.

Aurass, H.

Popow, E.

Oenel, H.

Dionies, F.

Bauer, S.

Rendtel, J.

Warmuth, A.

Woche, M.

Plueschke, D.

Bittner, W.

Paschke, J.

Wolter, D.

Van Beek, H. F.

Farnik, F.

机构：

[1] Univ Appl Sci & Arts NW Switzerland, Windisch, Switzerland

来源：

SPACE TELESCOPES AND INSTRUMENTATION 2012: ULTRAVIOLET TO GAMMA RAY | 2012年 / 8443卷

关键词：

X-ray imaging; X-ray spectrometer; Solar Physics;

D O I：

10.1117/12.927793

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The Spectrometer Telescope for Imaging X-rays (STIX) is one of 10 instruments on board Solar Orbiter, a confirmed M-class mission of the European Space Agency (ESA) within the Cosmic Vision program scheduled to be launched in 2017. STIX applies a Fourier-imaging technique using a set of tungsten grids (at pitches from 0.038 to 1 mm) in front of 32 pixelized CdTe detectors to provide imaging spectroscopy of solar thermal and non-thermal hard X-ray emissions from 4 to 150 keV. The status of the instrument reviewed in this paper is based on the design that passed the Preliminary Design Review (PDR) in early 2012. Particular emphasis is given to the first light of the detector system called Caliste-SO.

引用

页数：15

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