Performance of diamond detectors for VUV applications

被引:29
作者
BenMoussa, A.
Theissen, A.
Scholze, F.
Hochedez, J. F.
Schuehle, U.
Schmutz, W.
Haenen, K.
Stockman, Y.
Soltani, A.
McMullin, D.
Vest, R. E.
Kroth, U.
Laubis, C.
Richter, M.
Mortet, V.
Gissot, S.
Delouille, V.
Dominique, M.
Koller, S.
Halain, J. P.
Remes, Z.
Petersen, R.
D'Olieslaeger, M.
Defise, J. -M
机构
[1] Royal Observ Belgium, B-1180 Brussels, Belgium
[2] Phys Tech Bundesanstalt, Inst Berlin, D-10587 Berlin, Germany
[3] Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany
[4] Phys Meteorol Observ Davos, World Radiat Ctr, CH-7260 Davos, Switzerland
[5] Limburgs Univ Ctr, Inst Mat Res, B-3590 Diepenbeek, Belgium
[6] IMEC VZW, Div IMOMEC, B-3590 Diepenbeek, Belgium
[7] Ctr Spatial Liege, B-4031 Angleur, Belgium
[8] IEMN, F-59652 Villeneuve Dascq, France
[9] USN, Res Lab, Washington, DC 20375 USA
[10] Natl Inst Stand & Technol, Gaithersburg, MD 20899 USA
关键词
UV detectors; diamond; solar-blind photodetector;
D O I
10.1016/j.nima.2006.06.007
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
We report on experimental results with photodetectors made of diamond. the Large Yield Radiometer (LYRA), will use such detectors for the first time for a solar physics space instrument. A (LYRA) set of measurement campaigns was carried out to obtain their XUV-to-VIS characterization (responsivity, linearity, stability, homogeneity). The responsivity has been measured from the XUV to the NIR, in the wavelength range 1-1127 nm (i.e. 1240-1.1 eV). The diamond detectors exhibit a photoresponse varying in the 40-75 mA/W range at 7 nm and demonstrate a visible rejection ratio (200 versus 500 nm) larger than four orders of magnitude. We show that diamond photodetectors are sensitive sensors for VUV photons, stable within a few percent, with a good linearity and moderate homogeneity. (c) 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码:398 / 405
页数:8
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