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Title:
Performance of diamond detectors for VUV applications
Authors:
Benmoussa, A.; Theissen, A.; Scholze, F.; Hochedez, J. F.; Schühle, 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.
Affiliation:
AA(Royal Observatory of Belgium, Circular Avenue 3, B-1180 Brussels, Belgium), AB(Royal Observatory of Belgium, Circular Avenue 3, B-1180 Brussels, Belgium), AC(Physikalisch-Technische Bundesanstalt (PTB), Abbestr. 2-12, D-10587 Berlin, Germany), AD(Royal Observatory of Belgium, Circular Avenue 3, B-1180 Brussels, Belgium), AE(Max-Planck-Institut für Sonnensystemforschung, D-37191 Katlenburg-Lindau, Germany), AF(Physikalisch-Meteorologisches Observatorium Davos, World Radiation Center, CH-7260 Davos Dorf, Switzerland), AG(Institute for Materials Research, Limburgs Universitair Centrum, Wetenschapspark 1, B-3590 Diepenbeek, Belgium; Division IMOMEC, IMEC vzw, Wetenschapspark 1, B-3590 Diepenbeek, Belgium), AH(Centre Spatial de Liège, Av. Pré Aily B-4031 Angleur, Belgium), AI(Institut d'Electronique, de Microélectronique et de Nanotechnologie (IEMN) F-59652 Villeneuve d'Ascq, France), AJ(Naval Research Laboratory (NRL), 4555 Overlook Avenue, S.W., Washington, DC 20375, USA), AK(National Institute of Standards and Technology (NIST), 100 Bureau Drive, Gaithersburg, MD 20899, USA), AL(Physikalisch-Technische Bundesanstalt (PTB), Abbestr. 2-12, D-10587 Berlin, Germany), AM(Physikalisch-Technische Bundesanstalt (PTB), Abbestr. 2-12, D-10587 Berlin, Germany), AN(Physikalisch-Technische Bundesanstalt (PTB), Abbestr. 2-12, D-10587 Berlin, Germany), AO(Institute for Materials Research, Limburgs Universitair Centrum, Wetenschapspark 1, B-3590 Diepenbeek, Belgium), AP(Royal Observatory of Belgium, Circular Avenue 3, B-1180 Brussels, Belgium), AQ(Royal Observatory of Belgium, Circular Avenue 3, B-1180 Brussels, Belgium), AR(Royal Observatory of Belgium, Circular Avenue 3, B-1180 Brussels, Belgium), AS(Physikalisch-Meteorologisches Observatorium Davos, World Radiation Center, CH-7260 Davos Dorf, Switzerland), AT(Centre Spatial de Liège, Av. Pré Aily B-4031 Angleur, Belgium), AU(Institute for Materials Research, Limburgs Universitair Centrum, Wetenschapspark 1, B-3590 Diepenbeek, Belgium), AV(Division IMOMEC, IMEC vzw, Wetenschapspark 1, B-3590 Diepenbeek, Belgium), AW(Institute for Materials Research, Limburgs Universitair Centrum, Wetenschapspark 1, B-3590 Diepenbeek, Belgium; Division IMOMEC, IMEC vzw, Wetenschapspark 1, B-3590 Diepenbeek, Belgium), AX(Centre Spatial de Liège, Av. Pré Aily B-4031 Angleur, Belgium)
Publication:
Nuclear Instruments and Methods in Physics Research Section A, Volume 568, Issue 1, p. 398-405.
Publication Date:
11/2006
Origin:
ELSEVIER
PACS Keywords:
Photoconduction and photovoltaic effects
DOI:
10.1016/j.nima.2006.06.007
Bibliographic Code:
2006NIMPA.568..398B

Abstract

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.
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