Diamond detectors for LYRA, the solar VUV ...
Type de document :
Compte-rendu et recension critique d'ouvrage
Titre :
Diamond detectors for LYRA, the solar VUV radiometer on board PROBA2
Auteur(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]
Titre de la revue :
Diamond and Related Materials
Pagination :
802-806
Éditeur :
Elsevier
Date de publication :
2006
ISSN :
0925-9635
Mot(s)-clé(s) en anglais :
UV detectors
Diamond
Photodiode
Photoconductor
Diamond
Photodiode
Photoconductor
Discipline(s) HAL :
Planète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
Résumé en anglais : [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 ...
Lire la suite >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.Lire moins >
Lire la suite >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.Lire moins >
Langue :
Anglais
Vulgarisation :
Non
Source :
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