LYRA, a solar UV radiometer on Proba2
Document type :
Article dans une revue scientifique: Article original
Title :
LYRA, a solar UV radiometer on Proba2
Author(s) :
Hochedez, Jean-François [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Schmutz, W. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Stockman, Y. [Auteur]
Centre Spatial de Liège [CSL]
Schühle, U. [Auteur]
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Benmoussa, A. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Koller, S. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Haenen, K. [Auteur]
Istituto di Fisica dello Spazio Interplanetario [IFSI]
Institute for Materials Research [Diepenbeek]
Berghmans, D. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Defise, J.-M. [Auteur]
Centre Spatial de Liège [CSL]
Halain, J.-P. [Auteur]
Centre Spatial de Liège [CSL]
Theissen, A. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Delouille, V. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Slemzin, V. [Auteur]
P. N. Lebedev Physical Institute of the Russian Academy of Sciences [Moscow] [LPI RAS]
Gillotay, D. [Auteur]
Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique [BIRA-IASB]
Fussen, Didier [Auteur]
Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique [BIRA-IASB]
Dominique, M. [Auteur]
Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique [BIRA-IASB]
Vanhellemont, Filip [Auteur]
Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique [BIRA-IASB]
Mcmullin, D. [Auteur]
Naval Research Laboratory [NRL]
Kretzschmar, Matthieu [Auteur]
Istituto di Fisica dello Spazio Interplanetario [IFSI]
Mitrofanov, A. [Auteur]
P. N. Lebedev Physical Institute of the Russian Academy of Sciences [Moscow] [LPI RAS]
Nicula, B. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Wauters, L. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Roth, H. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Rozanov, E. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Rüedi, I. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Wehrli, C. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Soltani, Ali [Auteur]
Institut d’Électronique, de Microélectronique et de Nanotechnologie - UMR 8520 [IEMN]
Hamano, H. [Auteur]
van Der Linden, R. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Zhukov, A. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Clette, F. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Koizumi, S. [Auteur]
Mortet, V. [Auteur]
Institute for Materials Research [Diepenbeek]
Remes, Z. [Auteur]
Institute for Materials Research [Diepenbeek]
Petersen, R. [Auteur]
Interuniversity Microelectronics Centre - Institut de micro-électronique et composants [Belgique] [IMEC]
Nesladek, M. [Auteur]
Interuniversity Microelectronics Centre - Institut de micro-électronique et composants [Belgique] [IMEC]
Institute for Materials Research [Diepenbeek]
d'Olieslaeger, M. [Auteur]
Interuniversity Microelectronics Centre - Institut de micro-électronique et composants [Belgique] [IMEC]
Institute for Materials Research [Diepenbeek]
Roggen, J. [Auteur]
Interuniversity Microelectronics Centre - Institut de micro-électronique et composants [Belgique] [IMEC]
Rochus, P. [Auteur]
Centre Spatial de Liège [CSL]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Schmutz, W. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Stockman, Y. [Auteur]
Centre Spatial de Liège [CSL]
Schühle, U. [Auteur]
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Benmoussa, A. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Koller, S. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Haenen, K. [Auteur]
Istituto di Fisica dello Spazio Interplanetario [IFSI]
Institute for Materials Research [Diepenbeek]
Berghmans, D. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Defise, J.-M. [Auteur]
Centre Spatial de Liège [CSL]
Halain, J.-P. [Auteur]
Centre Spatial de Liège [CSL]
Theissen, A. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Delouille, V. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Slemzin, V. [Auteur]
P. N. Lebedev Physical Institute of the Russian Academy of Sciences [Moscow] [LPI RAS]
Gillotay, D. [Auteur]
Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique [BIRA-IASB]
Fussen, Didier [Auteur]
Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique [BIRA-IASB]
Dominique, M. [Auteur]
Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique [BIRA-IASB]
Vanhellemont, Filip [Auteur]
Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique [BIRA-IASB]
Mcmullin, D. [Auteur]
Naval Research Laboratory [NRL]
Kretzschmar, Matthieu [Auteur]
Istituto di Fisica dello Spazio Interplanetario [IFSI]
Mitrofanov, A. [Auteur]
P. N. Lebedev Physical Institute of the Russian Academy of Sciences [Moscow] [LPI RAS]
Nicula, B. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Wauters, L. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Roth, H. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Rozanov, E. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Rüedi, I. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Wehrli, C. [Auteur]
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center [PMOD/WRC]
Soltani, Ali [Auteur]

Institut d’Électronique, de Microélectronique et de Nanotechnologie - UMR 8520 [IEMN]
Hamano, H. [Auteur]
van Der Linden, R. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Zhukov, A. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Clette, F. [Auteur]
Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB]
Koizumi, S. [Auteur]
Mortet, V. [Auteur]
Institute for Materials Research [Diepenbeek]
Remes, Z. [Auteur]
Institute for Materials Research [Diepenbeek]
Petersen, R. [Auteur]
Interuniversity Microelectronics Centre - Institut de micro-électronique et composants [Belgique] [IMEC]
Nesladek, M. [Auteur]
Interuniversity Microelectronics Centre - Institut de micro-électronique et composants [Belgique] [IMEC]
Institute for Materials Research [Diepenbeek]
d'Olieslaeger, M. [Auteur]
Interuniversity Microelectronics Centre - Institut de micro-électronique et composants [Belgique] [IMEC]
Institute for Materials Research [Diepenbeek]
Roggen, J. [Auteur]
Interuniversity Microelectronics Centre - Institut de micro-électronique et composants [Belgique] [IMEC]
Rochus, P. [Auteur]
Centre Spatial de Liège [CSL]
Journal title :
Advances in Space Research
Pages :
303-312
Publisher :
Elsevier
Publication date :
2006
ISSN :
0273-1177
HAL domain(s) :
Planète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
English abstract : [en]
LYRA is the solar UV radiometer that will embark in 2006 onboard Proba2, a technologically oriented ESA micro-mission. LYRA is designed and manufactured by a Belgian–Swiss–German consortium (ROB, PMOD/WRC, IMOMEC, CSL, MPS ...
Show more >LYRA is the solar UV radiometer that will embark in 2006 onboard Proba2, a technologically oriented ESA micro-mission. LYRA is designed and manufactured by a Belgian–Swiss–German consortium (ROB, PMOD/WRC, IMOMEC, CSL, MPS and BISA) with additional international collaborations. It will monitor the solar irradiance in four UV passbands. They have been chosen for their relevance to Solar Physics, Aeronomy and Space Weather: (1) the 115–125 nm Lyman-α channel, (2) the 200–220 nm Herzberg continuum range, (3) the Aluminium filter channel (17–70 nm) including He II at 30.4 nm and (4) the Zirconium filter channel (1–20 nm). The radiometric calibration will be traceable to synchrotron source standards (PTB and NIST). The stability will be monitored by onboard calibration sources (LEDs), which allow to distinguish between potential degradations of the detectors and filters. Additionally, a redundancy strategy maximizes the accuracy and the stability of the measurements. LYRA will benefit from wide bandgap detectors based on diamond: it will be the first space assessment of a pioneering UV detectors program. Diamond sensors make the instruments radiation-hard and solar-blind: their high bandgap energy makes them insensitive to visible light and, therefore, make dispensable visible light blocking filters, which seriously attenuate the desired ultraviolet signal. Their elimination augments the effective area and hence the signal-to-noise, therefore increasing the precision and the cadence. The SWAP EUV imaging telescope will operate next to LYRA on Proba2. Together, they will establish a high performance solar monitor for operational space weather nowcasting and research. LYRA demonstrates technologies important for future missions such as the ESA Solar Orbiter.Show less >
Show more >LYRA is the solar UV radiometer that will embark in 2006 onboard Proba2, a technologically oriented ESA micro-mission. LYRA is designed and manufactured by a Belgian–Swiss–German consortium (ROB, PMOD/WRC, IMOMEC, CSL, MPS and BISA) with additional international collaborations. It will monitor the solar irradiance in four UV passbands. They have been chosen for their relevance to Solar Physics, Aeronomy and Space Weather: (1) the 115–125 nm Lyman-α channel, (2) the 200–220 nm Herzberg continuum range, (3) the Aluminium filter channel (17–70 nm) including He II at 30.4 nm and (4) the Zirconium filter channel (1–20 nm). The radiometric calibration will be traceable to synchrotron source standards (PTB and NIST). The stability will be monitored by onboard calibration sources (LEDs), which allow to distinguish between potential degradations of the detectors and filters. Additionally, a redundancy strategy maximizes the accuracy and the stability of the measurements. LYRA will benefit from wide bandgap detectors based on diamond: it will be the first space assessment of a pioneering UV detectors program. Diamond sensors make the instruments radiation-hard and solar-blind: their high bandgap energy makes them insensitive to visible light and, therefore, make dispensable visible light blocking filters, which seriously attenuate the desired ultraviolet signal. Their elimination augments the effective area and hence the signal-to-noise, therefore increasing the precision and the cadence. The SWAP EUV imaging telescope will operate next to LYRA on Proba2. Together, they will establish a high performance solar monitor for operational space weather nowcasting and research. LYRA demonstrates technologies important for future missions such as the ESA Solar Orbiter.Show less >
Language :
Anglais
Peer reviewed article :
Oui
Audience :
Non spécifiée
Popular science :
Non
Source :
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