SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission
Abstract The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Hori...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Cremonese, G. [verfasserIn] Capaccioni, F. [verfasserIn] Capria, M. T. [verfasserIn] Doressoundiram, A. [verfasserIn] Palumbo, P. [verfasserIn] Vincendon, M. [verfasserIn] Massironi, M. [verfasserIn] Debei, S. [verfasserIn] Zusi, M. [verfasserIn] Altieri, F. [verfasserIn] Amoroso, M. [verfasserIn] Aroldi, G. [verfasserIn] Baroni, M. [verfasserIn] Barucci, A. [verfasserIn] Bellucci, G. [verfasserIn] Benkhoff, J. [verfasserIn] Besse, S. [verfasserIn] Bettanini, C. [verfasserIn] Blecka, M. [verfasserIn] Borrelli, D. [verfasserIn] Brucato, J. R. [verfasserIn] Carli, C. [verfasserIn] Carlier, V. [verfasserIn] Cerroni, P. [verfasserIn] Cicchetti, A. [verfasserIn] Colangeli, L. [verfasserIn] Dami, M. [verfasserIn] Da Deppo, V. [verfasserIn] Della Corte, V. [verfasserIn] De Sanctis, M. C. [verfasserIn] Erard, S. [verfasserIn] Esposito, F. [verfasserIn] Fantinel, D. [verfasserIn] Ferranti, L. [verfasserIn] Ferri, F. [verfasserIn] Ficai Veltroni, I. [verfasserIn] Filacchione, G. [verfasserIn] Flamini, E. [verfasserIn] Forlani, G. [verfasserIn] Fornasier, S. [verfasserIn] Forni, O. [verfasserIn] Fulchignoni, M. [verfasserIn] Galluzzi, V. [verfasserIn] Gwinner, K. [verfasserIn] Ip, W. [verfasserIn] Jorda, L. [verfasserIn] Langevin, Y. [verfasserIn] Lara, L. [verfasserIn] Leblanc, F. [verfasserIn] Leyrat, C. [verfasserIn] Li, Y. [verfasserIn] Marchi, S. [verfasserIn] Marinangeli, L. [verfasserIn] Marzari, F. [verfasserIn] Mazzotta Epifani, E. [verfasserIn] Mendillo, M. [verfasserIn] Mennella, V. [verfasserIn] Mugnuolo, R. [verfasserIn] Muinonen, K. [verfasserIn] Naletto, G. [verfasserIn] Noschese, R. [verfasserIn] Palomba, E. [verfasserIn] Paolinetti, R. [verfasserIn] Perna, D. [verfasserIn] Piccioni, G. [verfasserIn] Politi, R. [verfasserIn] Poulet, F. [verfasserIn] Ragazzoni, R. [verfasserIn] Re, C. [verfasserIn] Rossi, M. [verfasserIn] Rotundi, A. [verfasserIn] Salemi, G. [verfasserIn] Sgavetti, M. [verfasserIn] Simioni, E. [verfasserIn] Thomas, N. [verfasserIn] Tommasi, L. [verfasserIn] Turella, A. [verfasserIn] Van Hoolst, T. [verfasserIn] Wilson, L. [verfasserIn] Zambon, F. [verfasserIn] Aboudan, A. [verfasserIn] Barraud, O. [verfasserIn] Bott, N. [verfasserIn] Borin, P. [verfasserIn] Colombatti, G. [verfasserIn] El Yazidi, M. [verfasserIn] Ferrari, S. [verfasserIn] Flahaut, J. [verfasserIn] Giacomini, L. [verfasserIn] Guzzetta, L. [verfasserIn] Lucchetti, A. [verfasserIn] Martellato, E. [verfasserIn] Pajola, M. [verfasserIn] Slemer, A. [verfasserIn] Tognon, G. [verfasserIn] Turrini, D. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2020 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962, 216(2020), 5 vom: 17. Juni |
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| Übergeordnetes Werk: |
volume:216 ; year:2020 ; number:5 ; day:17 ; month:06 |
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| DOI / URN: |
10.1007/s11214-020-00704-8 |
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| Katalog-ID: |
SPR040072339 |
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| 520 | |a Abstract The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well. | ||
| 650 | 4 | |a BepiColombo |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Mercury |7 (dpeaa)DE-He213 | |
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| 700 | 1 | |a Bellucci, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Benkhoff, J. |e verfasserin |4 aut | |
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| 700 | 1 | |a Bettanini, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Blecka, M. |e verfasserin |4 aut | |
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2020 |
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10.1007/s11214-020-00704-8 doi (DE-627)SPR040072339 (SPR)s11214-020-00704-8-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Cremonese, G. verfasserin aut SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well. BepiColombo (dpeaa)DE-He213 Mercury (dpeaa)DE-He213 Capaccioni, F. verfasserin aut Capria, M. T. verfasserin aut Doressoundiram, A. verfasserin aut Palumbo, P. verfasserin aut Vincendon, M. verfasserin aut Massironi, M. verfasserin aut Debei, S. verfasserin aut Zusi, M. verfasserin aut Altieri, F. verfasserin aut Amoroso, M. verfasserin aut Aroldi, G. verfasserin aut Baroni, M. verfasserin aut Barucci, A. verfasserin aut Bellucci, G. verfasserin aut Benkhoff, J. verfasserin aut Besse, S. verfasserin aut Bettanini, C. verfasserin aut Blecka, M. verfasserin aut Borrelli, D. verfasserin aut Brucato, J. R. verfasserin aut Carli, C. verfasserin aut Carlier, V. verfasserin aut Cerroni, P. verfasserin aut Cicchetti, A. verfasserin aut Colangeli, L. verfasserin aut Dami, M. verfasserin aut Da Deppo, V. verfasserin aut Della Corte, V. verfasserin aut De Sanctis, M. C. verfasserin aut Erard, S. verfasserin aut Esposito, F. verfasserin aut Fantinel, D. verfasserin aut Ferranti, L. verfasserin aut Ferri, F. verfasserin aut Ficai Veltroni, I. verfasserin aut Filacchione, G. verfasserin aut Flamini, E. verfasserin aut Forlani, G. verfasserin aut Fornasier, S. verfasserin aut Forni, O. verfasserin aut Fulchignoni, M. verfasserin aut Galluzzi, V. verfasserin aut Gwinner, K. verfasserin aut Ip, W. verfasserin aut Jorda, L. verfasserin aut Langevin, Y. verfasserin aut Lara, L. verfasserin aut Leblanc, F. verfasserin aut Leyrat, C. verfasserin aut Li, Y. verfasserin aut Marchi, S. verfasserin aut Marinangeli, L. verfasserin aut Marzari, F. verfasserin aut Mazzotta Epifani, E. verfasserin aut Mendillo, M. verfasserin aut Mennella, V. verfasserin aut Mugnuolo, R. verfasserin aut Muinonen, K. verfasserin aut Naletto, G. verfasserin aut Noschese, R. verfasserin aut Palomba, E. verfasserin aut Paolinetti, R. verfasserin aut Perna, D. verfasserin aut Piccioni, G. verfasserin aut Politi, R. verfasserin aut Poulet, F. verfasserin aut Ragazzoni, R. verfasserin aut Re, C. verfasserin aut Rossi, M. verfasserin aut Rotundi, A. verfasserin aut Salemi, G. verfasserin aut Sgavetti, M. verfasserin aut Simioni, E. verfasserin aut Thomas, N. verfasserin aut Tommasi, L. verfasserin aut Turella, A. verfasserin aut Van Hoolst, T. verfasserin aut Wilson, L. verfasserin aut Zambon, F. verfasserin aut Aboudan, A. verfasserin aut Barraud, O. verfasserin aut Bott, N. verfasserin aut Borin, P. verfasserin aut Colombatti, G. verfasserin aut El Yazidi, M. verfasserin aut Ferrari, S. verfasserin aut Flahaut, J. verfasserin aut Giacomini, L. verfasserin aut Guzzetta, L. verfasserin aut Lucchetti, A. verfasserin aut Martellato, E. verfasserin aut Pajola, M. verfasserin aut Slemer, A. verfasserin aut Tognon, G. verfasserin aut Turrini, D. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 216(2020), 5 vom: 17. Juni (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:216 year:2020 number:5 day:17 month:06 https://dx.doi.org/10.1007/s11214-020-00704-8 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 216 2020 5 17 06 |
| spelling |
10.1007/s11214-020-00704-8 doi (DE-627)SPR040072339 (SPR)s11214-020-00704-8-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Cremonese, G. verfasserin aut SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well. BepiColombo (dpeaa)DE-He213 Mercury (dpeaa)DE-He213 Capaccioni, F. verfasserin aut Capria, M. T. verfasserin aut Doressoundiram, A. verfasserin aut Palumbo, P. verfasserin aut Vincendon, M. verfasserin aut Massironi, M. verfasserin aut Debei, S. verfasserin aut Zusi, M. verfasserin aut Altieri, F. verfasserin aut Amoroso, M. verfasserin aut Aroldi, G. verfasserin aut Baroni, M. verfasserin aut Barucci, A. verfasserin aut Bellucci, G. verfasserin aut Benkhoff, J. verfasserin aut Besse, S. verfasserin aut Bettanini, C. verfasserin aut Blecka, M. verfasserin aut Borrelli, D. verfasserin aut Brucato, J. R. verfasserin aut Carli, C. verfasserin aut Carlier, V. verfasserin aut Cerroni, P. verfasserin aut Cicchetti, A. verfasserin aut Colangeli, L. verfasserin aut Dami, M. verfasserin aut Da Deppo, V. verfasserin aut Della Corte, V. verfasserin aut De Sanctis, M. C. verfasserin aut Erard, S. verfasserin aut Esposito, F. verfasserin aut Fantinel, D. verfasserin aut Ferranti, L. verfasserin aut Ferri, F. verfasserin aut Ficai Veltroni, I. verfasserin aut Filacchione, G. verfasserin aut Flamini, E. verfasserin aut Forlani, G. verfasserin aut Fornasier, S. verfasserin aut Forni, O. verfasserin aut Fulchignoni, M. verfasserin aut Galluzzi, V. verfasserin aut Gwinner, K. verfasserin aut Ip, W. verfasserin aut Jorda, L. verfasserin aut Langevin, Y. verfasserin aut Lara, L. verfasserin aut Leblanc, F. verfasserin aut Leyrat, C. verfasserin aut Li, Y. verfasserin aut Marchi, S. verfasserin aut Marinangeli, L. verfasserin aut Marzari, F. verfasserin aut Mazzotta Epifani, E. verfasserin aut Mendillo, M. verfasserin aut Mennella, V. verfasserin aut Mugnuolo, R. verfasserin aut Muinonen, K. verfasserin aut Naletto, G. verfasserin aut Noschese, R. verfasserin aut Palomba, E. verfasserin aut Paolinetti, R. verfasserin aut Perna, D. verfasserin aut Piccioni, G. verfasserin aut Politi, R. verfasserin aut Poulet, F. verfasserin aut Ragazzoni, R. verfasserin aut Re, C. verfasserin aut Rossi, M. verfasserin aut Rotundi, A. verfasserin aut Salemi, G. verfasserin aut Sgavetti, M. verfasserin aut Simioni, E. verfasserin aut Thomas, N. verfasserin aut Tommasi, L. verfasserin aut Turella, A. verfasserin aut Van Hoolst, T. verfasserin aut Wilson, L. verfasserin aut Zambon, F. verfasserin aut Aboudan, A. verfasserin aut Barraud, O. verfasserin aut Bott, N. verfasserin aut Borin, P. verfasserin aut Colombatti, G. verfasserin aut El Yazidi, M. verfasserin aut Ferrari, S. verfasserin aut Flahaut, J. verfasserin aut Giacomini, L. verfasserin aut Guzzetta, L. verfasserin aut Lucchetti, A. verfasserin aut Martellato, E. verfasserin aut Pajola, M. verfasserin aut Slemer, A. verfasserin aut Tognon, G. verfasserin aut Turrini, D. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 216(2020), 5 vom: 17. Juni (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:216 year:2020 number:5 day:17 month:06 https://dx.doi.org/10.1007/s11214-020-00704-8 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 216 2020 5 17 06 |
| allfields_unstemmed |
10.1007/s11214-020-00704-8 doi (DE-627)SPR040072339 (SPR)s11214-020-00704-8-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Cremonese, G. verfasserin aut SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well. BepiColombo (dpeaa)DE-He213 Mercury (dpeaa)DE-He213 Capaccioni, F. verfasserin aut Capria, M. T. verfasserin aut Doressoundiram, A. verfasserin aut Palumbo, P. verfasserin aut Vincendon, M. verfasserin aut Massironi, M. verfasserin aut Debei, S. verfasserin aut Zusi, M. verfasserin aut Altieri, F. verfasserin aut Amoroso, M. verfasserin aut Aroldi, G. verfasserin aut Baroni, M. verfasserin aut Barucci, A. verfasserin aut Bellucci, G. verfasserin aut Benkhoff, J. verfasserin aut Besse, S. verfasserin aut Bettanini, C. verfasserin aut Blecka, M. verfasserin aut Borrelli, D. verfasserin aut Brucato, J. R. verfasserin aut Carli, C. verfasserin aut Carlier, V. verfasserin aut Cerroni, P. verfasserin aut Cicchetti, A. verfasserin aut Colangeli, L. verfasserin aut Dami, M. verfasserin aut Da Deppo, V. verfasserin aut Della Corte, V. verfasserin aut De Sanctis, M. C. verfasserin aut Erard, S. verfasserin aut Esposito, F. verfasserin aut Fantinel, D. verfasserin aut Ferranti, L. verfasserin aut Ferri, F. verfasserin aut Ficai Veltroni, I. verfasserin aut Filacchione, G. verfasserin aut Flamini, E. verfasserin aut Forlani, G. verfasserin aut Fornasier, S. verfasserin aut Forni, O. verfasserin aut Fulchignoni, M. verfasserin aut Galluzzi, V. verfasserin aut Gwinner, K. verfasserin aut Ip, W. verfasserin aut Jorda, L. verfasserin aut Langevin, Y. verfasserin aut Lara, L. verfasserin aut Leblanc, F. verfasserin aut Leyrat, C. verfasserin aut Li, Y. verfasserin aut Marchi, S. verfasserin aut Marinangeli, L. verfasserin aut Marzari, F. verfasserin aut Mazzotta Epifani, E. verfasserin aut Mendillo, M. verfasserin aut Mennella, V. verfasserin aut Mugnuolo, R. verfasserin aut Muinonen, K. verfasserin aut Naletto, G. verfasserin aut Noschese, R. verfasserin aut Palomba, E. verfasserin aut Paolinetti, R. verfasserin aut Perna, D. verfasserin aut Piccioni, G. verfasserin aut Politi, R. verfasserin aut Poulet, F. verfasserin aut Ragazzoni, R. verfasserin aut Re, C. verfasserin aut Rossi, M. verfasserin aut Rotundi, A. verfasserin aut Salemi, G. verfasserin aut Sgavetti, M. verfasserin aut Simioni, E. verfasserin aut Thomas, N. verfasserin aut Tommasi, L. verfasserin aut Turella, A. verfasserin aut Van Hoolst, T. verfasserin aut Wilson, L. verfasserin aut Zambon, F. verfasserin aut Aboudan, A. verfasserin aut Barraud, O. verfasserin aut Bott, N. verfasserin aut Borin, P. verfasserin aut Colombatti, G. verfasserin aut El Yazidi, M. verfasserin aut Ferrari, S. verfasserin aut Flahaut, J. verfasserin aut Giacomini, L. verfasserin aut Guzzetta, L. verfasserin aut Lucchetti, A. verfasserin aut Martellato, E. verfasserin aut Pajola, M. verfasserin aut Slemer, A. verfasserin aut Tognon, G. verfasserin aut Turrini, D. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 216(2020), 5 vom: 17. Juni (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:216 year:2020 number:5 day:17 month:06 https://dx.doi.org/10.1007/s11214-020-00704-8 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 216 2020 5 17 06 |
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10.1007/s11214-020-00704-8 doi (DE-627)SPR040072339 (SPR)s11214-020-00704-8-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Cremonese, G. verfasserin aut SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well. BepiColombo (dpeaa)DE-He213 Mercury (dpeaa)DE-He213 Capaccioni, F. verfasserin aut Capria, M. T. verfasserin aut Doressoundiram, A. verfasserin aut Palumbo, P. verfasserin aut Vincendon, M. verfasserin aut Massironi, M. verfasserin aut Debei, S. verfasserin aut Zusi, M. verfasserin aut Altieri, F. verfasserin aut Amoroso, M. verfasserin aut Aroldi, G. verfasserin aut Baroni, M. verfasserin aut Barucci, A. verfasserin aut Bellucci, G. verfasserin aut Benkhoff, J. verfasserin aut Besse, S. verfasserin aut Bettanini, C. verfasserin aut Blecka, M. verfasserin aut Borrelli, D. verfasserin aut Brucato, J. R. verfasserin aut Carli, C. verfasserin aut Carlier, V. verfasserin aut Cerroni, P. verfasserin aut Cicchetti, A. verfasserin aut Colangeli, L. verfasserin aut Dami, M. verfasserin aut Da Deppo, V. verfasserin aut Della Corte, V. verfasserin aut De Sanctis, M. C. verfasserin aut Erard, S. verfasserin aut Esposito, F. verfasserin aut Fantinel, D. verfasserin aut Ferranti, L. verfasserin aut Ferri, F. verfasserin aut Ficai Veltroni, I. verfasserin aut Filacchione, G. verfasserin aut Flamini, E. verfasserin aut Forlani, G. verfasserin aut Fornasier, S. verfasserin aut Forni, O. verfasserin aut Fulchignoni, M. verfasserin aut Galluzzi, V. verfasserin aut Gwinner, K. verfasserin aut Ip, W. verfasserin aut Jorda, L. verfasserin aut Langevin, Y. verfasserin aut Lara, L. verfasserin aut Leblanc, F. verfasserin aut Leyrat, C. verfasserin aut Li, Y. verfasserin aut Marchi, S. verfasserin aut Marinangeli, L. verfasserin aut Marzari, F. verfasserin aut Mazzotta Epifani, E. verfasserin aut Mendillo, M. verfasserin aut Mennella, V. verfasserin aut Mugnuolo, R. verfasserin aut Muinonen, K. verfasserin aut Naletto, G. verfasserin aut Noschese, R. verfasserin aut Palomba, E. verfasserin aut Paolinetti, R. verfasserin aut Perna, D. verfasserin aut Piccioni, G. verfasserin aut Politi, R. verfasserin aut Poulet, F. verfasserin aut Ragazzoni, R. verfasserin aut Re, C. verfasserin aut Rossi, M. verfasserin aut Rotundi, A. verfasserin aut Salemi, G. verfasserin aut Sgavetti, M. verfasserin aut Simioni, E. verfasserin aut Thomas, N. verfasserin aut Tommasi, L. verfasserin aut Turella, A. verfasserin aut Van Hoolst, T. verfasserin aut Wilson, L. verfasserin aut Zambon, F. verfasserin aut Aboudan, A. verfasserin aut Barraud, O. verfasserin aut Bott, N. verfasserin aut Borin, P. verfasserin aut Colombatti, G. verfasserin aut El Yazidi, M. verfasserin aut Ferrari, S. verfasserin aut Flahaut, J. verfasserin aut Giacomini, L. verfasserin aut Guzzetta, L. verfasserin aut Lucchetti, A. verfasserin aut Martellato, E. verfasserin aut Pajola, M. verfasserin aut Slemer, A. verfasserin aut Tognon, G. verfasserin aut Turrini, D. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 216(2020), 5 vom: 17. Juni (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:216 year:2020 number:5 day:17 month:06 https://dx.doi.org/10.1007/s11214-020-00704-8 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 216 2020 5 17 06 |
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10.1007/s11214-020-00704-8 doi (DE-627)SPR040072339 (SPR)s11214-020-00704-8-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Cremonese, G. verfasserin aut SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well. BepiColombo (dpeaa)DE-He213 Mercury (dpeaa)DE-He213 Capaccioni, F. verfasserin aut Capria, M. T. verfasserin aut Doressoundiram, A. verfasserin aut Palumbo, P. verfasserin aut Vincendon, M. verfasserin aut Massironi, M. verfasserin aut Debei, S. verfasserin aut Zusi, M. verfasserin aut Altieri, F. verfasserin aut Amoroso, M. verfasserin aut Aroldi, G. verfasserin aut Baroni, M. verfasserin aut Barucci, A. verfasserin aut Bellucci, G. verfasserin aut Benkhoff, J. verfasserin aut Besse, S. verfasserin aut Bettanini, C. verfasserin aut Blecka, M. verfasserin aut Borrelli, D. verfasserin aut Brucato, J. R. verfasserin aut Carli, C. verfasserin aut Carlier, V. verfasserin aut Cerroni, P. verfasserin aut Cicchetti, A. verfasserin aut Colangeli, L. verfasserin aut Dami, M. verfasserin aut Da Deppo, V. verfasserin aut Della Corte, V. verfasserin aut De Sanctis, M. C. verfasserin aut Erard, S. verfasserin aut Esposito, F. verfasserin aut Fantinel, D. verfasserin aut Ferranti, L. verfasserin aut Ferri, F. verfasserin aut Ficai Veltroni, I. verfasserin aut Filacchione, G. verfasserin aut Flamini, E. verfasserin aut Forlani, G. verfasserin aut Fornasier, S. verfasserin aut Forni, O. verfasserin aut Fulchignoni, M. verfasserin aut Galluzzi, V. verfasserin aut Gwinner, K. verfasserin aut Ip, W. verfasserin aut Jorda, L. verfasserin aut Langevin, Y. verfasserin aut Lara, L. verfasserin aut Leblanc, F. verfasserin aut Leyrat, C. verfasserin aut Li, Y. verfasserin aut Marchi, S. verfasserin aut Marinangeli, L. verfasserin aut Marzari, F. verfasserin aut Mazzotta Epifani, E. verfasserin aut Mendillo, M. verfasserin aut Mennella, V. verfasserin aut Mugnuolo, R. verfasserin aut Muinonen, K. verfasserin aut Naletto, G. verfasserin aut Noschese, R. verfasserin aut Palomba, E. verfasserin aut Paolinetti, R. verfasserin aut Perna, D. verfasserin aut Piccioni, G. verfasserin aut Politi, R. verfasserin aut Poulet, F. verfasserin aut Ragazzoni, R. verfasserin aut Re, C. verfasserin aut Rossi, M. verfasserin aut Rotundi, A. verfasserin aut Salemi, G. verfasserin aut Sgavetti, M. verfasserin aut Simioni, E. verfasserin aut Thomas, N. verfasserin aut Tommasi, L. verfasserin aut Turella, A. verfasserin aut Van Hoolst, T. verfasserin aut Wilson, L. verfasserin aut Zambon, F. verfasserin aut Aboudan, A. verfasserin aut Barraud, O. verfasserin aut Bott, N. verfasserin aut Borin, P. verfasserin aut Colombatti, G. verfasserin aut El Yazidi, M. verfasserin aut Ferrari, S. verfasserin aut Flahaut, J. verfasserin aut Giacomini, L. verfasserin aut Guzzetta, L. verfasserin aut Lucchetti, A. verfasserin aut Martellato, E. verfasserin aut Pajola, M. verfasserin aut Slemer, A. verfasserin aut Tognon, G. verfasserin aut Turrini, D. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 216(2020), 5 vom: 17. Juni (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:216 year:2020 number:5 day:17 month:06 https://dx.doi.org/10.1007/s11214-020-00704-8 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 216 2020 5 17 06 |
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Space science reviews |
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Cremonese, G. @@aut@@ Capaccioni, F. @@aut@@ Capria, M. T. @@aut@@ Doressoundiram, A. @@aut@@ Palumbo, P. @@aut@@ Vincendon, M. @@aut@@ Massironi, M. @@aut@@ Debei, S. @@aut@@ Zusi, M. @@aut@@ Altieri, F. @@aut@@ Amoroso, M. @@aut@@ Aroldi, G. @@aut@@ Baroni, M. @@aut@@ Barucci, A. @@aut@@ Bellucci, G. @@aut@@ Benkhoff, J. @@aut@@ Besse, S. @@aut@@ Bettanini, C. @@aut@@ Blecka, M. @@aut@@ Borrelli, D. @@aut@@ Brucato, J. R. @@aut@@ Carli, C. @@aut@@ Carlier, V. @@aut@@ Cerroni, P. @@aut@@ Cicchetti, A. @@aut@@ Colangeli, L. @@aut@@ Dami, M. @@aut@@ Da Deppo, V. @@aut@@ Della Corte, V. @@aut@@ De Sanctis, M. C. @@aut@@ Erard, S. @@aut@@ Esposito, F. @@aut@@ Fantinel, D. @@aut@@ Ferranti, L. @@aut@@ Ferri, F. @@aut@@ Ficai Veltroni, I. @@aut@@ Filacchione, G. @@aut@@ Flamini, E. @@aut@@ Forlani, G. @@aut@@ Fornasier, S. @@aut@@ Forni, O. @@aut@@ Fulchignoni, M. @@aut@@ Galluzzi, V. @@aut@@ Gwinner, K. @@aut@@ Ip, W. @@aut@@ Jorda, L. @@aut@@ Langevin, Y. @@aut@@ Lara, L. @@aut@@ Leblanc, F. @@aut@@ Leyrat, C. @@aut@@ Li, Y. @@aut@@ Marchi, S. @@aut@@ Marinangeli, L. @@aut@@ Marzari, F. @@aut@@ Mazzotta Epifani, E. @@aut@@ Mendillo, M. @@aut@@ Mennella, V. @@aut@@ Mugnuolo, R. @@aut@@ Muinonen, K. @@aut@@ Naletto, G. @@aut@@ Noschese, R. @@aut@@ Palomba, E. @@aut@@ Paolinetti, R. @@aut@@ Perna, D. @@aut@@ Piccioni, G. @@aut@@ Politi, R. @@aut@@ Poulet, F. @@aut@@ Ragazzoni, R. @@aut@@ Re, C. @@aut@@ Rossi, M. @@aut@@ Rotundi, A. @@aut@@ Salemi, G. @@aut@@ Sgavetti, M. @@aut@@ Simioni, E. @@aut@@ Thomas, N. @@aut@@ Tommasi, L. @@aut@@ Turella, A. @@aut@@ Van Hoolst, T. @@aut@@ Wilson, L. @@aut@@ Zambon, F. @@aut@@ Aboudan, A. @@aut@@ Barraud, O. @@aut@@ Bott, N. @@aut@@ Borin, P. @@aut@@ Colombatti, G. @@aut@@ El Yazidi, M. @@aut@@ Ferrari, S. @@aut@@ Flahaut, J. @@aut@@ Giacomini, L. @@aut@@ Guzzetta, L. @@aut@@ Lucchetti, A. @@aut@@ Martellato, E. @@aut@@ Pajola, M. @@aut@@ Slemer, A. @@aut@@ Tognon, G. @@aut@@ Turrini, D. @@aut@@ |
| publishDateDaySort_date |
2020-06-17T00:00:00Z |
| hierarchy_top_id |
315621222 |
| dewey-sort |
3600 |
| id |
SPR040072339 |
| language_de |
englisch |
| fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR040072339</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220111053831.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">201007s2020 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11214-020-00704-8</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR040072339</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s11214-020-00704-8-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">600</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">39.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Cremonese, G.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2020</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">BepiColombo</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Mercury</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Capaccioni, F.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Capria, M. 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Cremonese, G. |
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Cremonese, G. ddc 600 bkl 39.00 misc BepiColombo misc Mercury SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission |
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600 ASE 39.00 bkl SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission BepiColombo (dpeaa)DE-He213 Mercury (dpeaa)DE-He213 |
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SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission |
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SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission |
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Cremonese, G. Capaccioni, F. Capria, M. T. Doressoundiram, A. Palumbo, P. Vincendon, M. Massironi, M. Debei, S. Zusi, M. Altieri, F. Amoroso, M. Aroldi, G. Baroni, M. Barucci, A. Bellucci, G. Benkhoff, J. Besse, S. Bettanini, C. Blecka, M. Borrelli, D. Brucato, J. R. Carli, C. Carlier, V. Cerroni, P. Cicchetti, A. Colangeli, L. Dami, M. Da Deppo, V. Della Corte, V. De Sanctis, M. C. Erard, S. Esposito, F. Fantinel, D. Ferranti, L. Ferri, F. Ficai Veltroni, I. Filacchione, G. Flamini, E. Forlani, G. Fornasier, S. Forni, O. Fulchignoni, M. Galluzzi, V. Gwinner, K. Ip, W. Jorda, L. Langevin, Y. Lara, L. Leblanc, F. Leyrat, C. Li, Y. Marchi, S. Marinangeli, L. Marzari, F. Mazzotta Epifani, E. Mendillo, M. Mennella, V. Mugnuolo, R. Muinonen, K. Naletto, G. Noschese, R. Palomba, E. Paolinetti, R. Perna, D. Piccioni, G. Politi, R. Poulet, F. Ragazzoni, R. Re, C. Rossi, M. Rotundi, A. Salemi, G. Sgavetti, M. Simioni, E. Thomas, N. Tommasi, L. Turella, A. Van Hoolst, T. Wilson, L. Zambon, F. Aboudan, A. Barraud, O. Bott, N. Borin, P. Colombatti, G. El Yazidi, M. Ferrari, S. Flahaut, J. Giacomini, L. Guzzetta, L. Lucchetti, A. Martellato, E. Pajola, M. Slemer, A. Tognon, G. Turrini, D. |
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Cremonese, G. |
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10.1007/s11214-020-00704-8 |
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simbio-sys: scientific cameras and spectrometer for the bepicolombo mission |
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SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission |
| abstract |
Abstract The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well. |
| abstractGer |
Abstract The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well. |
| abstract_unstemmed |
Abstract The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well. |
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| title_short |
SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission |
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https://dx.doi.org/10.1007/s11214-020-00704-8 |
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Capaccioni, F. Capria, M. T. Doressoundiram, A. Palumbo, P. Vincendon, M. Massironi, M. Debei, S. Zusi, M. Altieri, F. Amoroso, M. Aroldi, G. Baroni, M. Barucci, A. Bellucci, G. Benkhoff, J. Besse, S. Bettanini, C. Blecka, M. Borrelli, D. Brucato, J. R. Carli, C. Carlier, V. Cerroni, P. Cicchetti, A. Colangeli, L. Dami, M. Da Deppo, V. Della Corte, V. De Sanctis, M. C. Erard, S. Esposito, F. Fantinel, D. Ferranti, L. Ferri, F. Ficai Veltroni, I. Filacchione, G. Flamini, E. Forlani, G. Fornasier, S. Forni, O. Fulchignoni, M. Galluzzi, V. Gwinner, K. Ip, W. Jorda, L. Langevin, Y. Lara, L. Leblanc, F. Leyrat, C. Li, Y. Marchi, S. Marinangeli, L. Marzari, F. Mazzotta Epifani, E. Mendillo, M. Mennella, V. Mugnuolo, R. Muinonen, K. Naletto, G. Noschese, R. Palomba, E. Paolinetti, R. Perna, D. Piccioni, G. Politi, R. Poulet, F. Ragazzoni, R. Re, C. Rossi, M. Rotundi, A. Salemi, G. Sgavetti, M. Simioni, E. Thomas, N. Tommasi, L. Turella, A. Van Hoolst, T. Wilson, L. Zambon, F. Aboudan, A. Barraud, O. Bott, N. Borin, P. Colombatti, G. El Yazidi, M. Ferrari, S. Flahaut, J. Giacomini, L. Guzzetta, L. Lucchetti, A. Martellato, E. Pajola, M. Slemer, A. Tognon, G. Turrini, D. |
| author2Str |
Capaccioni, F. Capria, M. T. Doressoundiram, A. Palumbo, P. Vincendon, M. Massironi, M. Debei, S. Zusi, M. Altieri, F. Amoroso, M. Aroldi, G. Baroni, M. Barucci, A. Bellucci, G. Benkhoff, J. Besse, S. Bettanini, C. Blecka, M. Borrelli, D. Brucato, J. R. Carli, C. Carlier, V. Cerroni, P. Cicchetti, A. Colangeli, L. Dami, M. Da Deppo, V. Della Corte, V. De Sanctis, M. C. Erard, S. Esposito, F. Fantinel, D. Ferranti, L. Ferri, F. Ficai Veltroni, I. Filacchione, G. Flamini, E. Forlani, G. Fornasier, S. Forni, O. Fulchignoni, M. Galluzzi, V. Gwinner, K. Ip, W. Jorda, L. Langevin, Y. Lara, L. Leblanc, F. Leyrat, C. Li, Y. Marchi, S. Marinangeli, L. Marzari, F. Mazzotta Epifani, E. Mendillo, M. Mennella, V. Mugnuolo, R. Muinonen, K. Naletto, G. Noschese, R. Palomba, E. Paolinetti, R. Perna, D. Piccioni, G. Politi, R. Poulet, F. Ragazzoni, R. Re, C. Rossi, M. Rotundi, A. Salemi, G. Sgavetti, M. Simioni, E. Thomas, N. Tommasi, L. Turella, A. Van Hoolst, T. Wilson, L. Zambon, F. Aboudan, A. Barraud, O. Bott, N. Borin, P. Colombatti, G. El Yazidi, M. Ferrari, S. Flahaut, J. Giacomini, L. Guzzetta, L. Lucchetti, A. Martellato, E. Pajola, M. Slemer, A. Tognon, G. Turrini, D. |
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| doi_str |
10.1007/s11214-020-00704-8 |
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2024-07-03T13:36:58.678Z |
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|
| score |
7.399515 |