Diamond detectors for LYRA, the solar VUV ...
Document type :
Compte-rendu et recension critique d'ouvrage
Title :
Diamond detectors for LYRA, the solar VUV radiometer on board PROBA2
Author(s) :
Benmoussa, A. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Hochedez, Jean-François [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Schühle, U. [Auteur]
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Schmutz, W. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Haenen, K. [Auteur]
Institute for Materials Research [Diepenbeek]
Stockman, Y. [Auteur]
Centre Spatial de Liège [CSL]
Soltani, Ali [Auteur]
Institut d’Électronique, de Microélectronique et de Nanotechnologie - UMR 8520 [IEMN]
Scholze, F. [Auteur]
Physikalisch-Technische Bundesanstalt [Berlin] [PTB]
Kroth, U. [Auteur]
Physikalisch-Technische Bundesanstalt [Berlin] [PTB]
Mortet, V. [Auteur]
Institute for Materials Research [Diepenbeek]
Theissen, A. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Laubis, C. [Auteur]
Physikalisch-Technische Bundesanstalt [Berlin] [PTB]
Richter, M. [Auteur]
Physikalisch-Technische Bundesanstalt [Berlin] [PTB]
Kollerc, S. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Defise, J.M. [Auteur]
Centre Spatial de Liège [CSL]
Koizumi, S. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Hochedez, Jean-François [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Schühle, U. [Auteur]
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Schmutz, W. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Haenen, K. [Auteur]
Institute for Materials Research [Diepenbeek]
Stockman, Y. [Auteur]
Centre Spatial de Liège [CSL]
Soltani, Ali [Auteur]
Institut d’Électronique, de Microélectronique et de Nanotechnologie - UMR 8520 [IEMN]
Scholze, F. [Auteur]
Physikalisch-Technische Bundesanstalt [Berlin] [PTB]
Kroth, U. [Auteur]
Physikalisch-Technische Bundesanstalt [Berlin] [PTB]
Mortet, V. [Auteur]
Institute for Materials Research [Diepenbeek]
Theissen, A. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Laubis, C. [Auteur]
Physikalisch-Technische Bundesanstalt [Berlin] [PTB]
Richter, M. [Auteur]
Physikalisch-Technische Bundesanstalt [Berlin] [PTB]
Kollerc, S. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Defise, J.M. [Auteur]
Centre Spatial de Liège [CSL]
Koizumi, S. [Auteur]
Journal title :
Diamond and Related Materials
Pages :
802-806
Publisher :
Elsevier
Publication date :
2006
ISSN :
0925-9635
English keyword(s) :
UV detectors
Diamond
Photodiode
Photoconductor
Diamond
Photodiode
Photoconductor
HAL domain(s) :
Planète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
English abstract : [en]
New pin-photodiode and metal–semiconductor–metal (MSM) photoconductor devices based on diamond material have been produced showing high responsivity around 200 nm. LYRA, the Large Yield RAdiometer, will use such detectors ...
Show more >New pin-photodiode and metal–semiconductor–metal (MSM) photoconductor devices based on diamond material have been produced showing high responsivity around 200 nm. LYRA, the Large Yield RAdiometer, will use such detectors for the first time for a solar physics space instrument. A set of measurement campaigns was carried out to obtain their XUV-to-VIS characterization (responsivity, linearity, stability and homogeneity). The diamond pin and MSM photodetectors exhibit a high responsivity of 27 mA/W around 200 nm and demonstrate a visible rejection ratio (200 nm versus 500 nm) of six and four orders of magnitude, respectively. We show that these diamond photodetectors are sensitive sensors for the wavelength range of interest (1 nm to 220 nm), stable within a few percent, with a good linearity and moderate homogeneity.Show less >
Show more >New pin-photodiode and metal–semiconductor–metal (MSM) photoconductor devices based on diamond material have been produced showing high responsivity around 200 nm. LYRA, the Large Yield RAdiometer, will use such detectors for the first time for a solar physics space instrument. A set of measurement campaigns was carried out to obtain their XUV-to-VIS characterization (responsivity, linearity, stability and homogeneity). The diamond pin and MSM photodetectors exhibit a high responsivity of 27 mA/W around 200 nm and demonstrate a visible rejection ratio (200 nm versus 500 nm) of six and four orders of magnitude, respectively. We show that these diamond photodetectors are sensitive sensors for the wavelength range of interest (1 nm to 220 nm), stable within a few percent, with a good linearity and moderate homogeneity.Show less >
Language :
Anglais
Popular science :
Non
Source :
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