SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo
Abstract The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interpl...
Ausführliche Beschreibung
Autor*in: |
Orsini, S. [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
2021 |
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Schlagwörter: |
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Anmerkung: |
© The Author(s) 2021. corrected publication 2021 |
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Übergeordnetes Werk: |
Enthalten in: Space science reviews - Springer Netherlands, 1962, 217(2021), 1 vom: 12. Jan. |
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Übergeordnetes Werk: |
volume:217 ; year:2021 ; number:1 ; day:12 ; month:01 |
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DOI / URN: |
10.1007/s11214-020-00787-3 |
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OLC2122641215 |
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520 | |a Abstract The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase. | ||
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650 | 4 | |a Particle instrumentation | |
650 | 4 | |a BepiColombo space mission | |
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700 | 1 | |a Lichtenegger, H. |4 aut | |
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700 | 1 | |a Milillo, A. |4 aut | |
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700 | 1 | |a Phillips, M. |4 aut | |
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700 | 1 | |a Szego, K. |4 aut | |
700 | 1 | |a Aronica, A. |4 aut | |
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700 | 1 | |a Di Lellis, A. M. |4 aut | |
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10.1007/s11214-020-00787-3 doi (DE-627)OLC2122641215 (DE-He213)s11214-020-00787-3-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Orsini, S. verfasserin aut SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021. corrected publication 2021 Abstract The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase. Mercury’s environment Particle instrumentation BepiColombo space mission Livi, S. A. aut Lichtenegger, H. aut Barabash, S. aut Milillo, A. aut De Angelis, E. aut Phillips, M. aut Laky, G. aut Wieser, M. aut Olivieri, A. aut Plainaki, C. aut Ho, G. aut Killen, R. M. aut Slavin, J. A. aut Wurz, P. aut Berthelier, J.-J. aut Dandouras, I. aut Kallio, E. aut McKenna-Lawlor, S. aut Szalai, S. aut Torkar, K. aut Vaisberg, O. aut Allegrini, F. aut Daglis, I. A. aut Dong, C. aut Escoubet, C. P. aut Fatemi, S. aut Fränz, M. aut Ivanovski, S. aut Krupp, N. aut Lammer, H. aut Leblanc, François aut Mangano, V. aut Mura, A. aut Nilsson, H. aut Raines, J. M. aut Rispoli, R. aut Sarantos, M. aut Smith, H. T. aut Szego, K. aut Aronica, A. aut Camozzi, F. aut Di Lellis, A. M. aut Fremuth, G. aut Giner, F. aut Gurnee, R. aut Hayes, J. aut Jeszenszky, H. aut Tominetti, F. aut Trantham, B. aut Balaz, J. aut Baumjohann, W. aut Brienza, D. aut Bührke, U. aut Bush, M. D. aut Cantatore, M. aut Cibella, S. aut Colasanti, L. aut Cremonese, G. aut Cremonesi, L. aut D’Alessandro, M. aut Delcourt, D. aut Delva, M. aut Desai, M. aut Fama, M. aut Ferris, M. aut Fischer, H. aut Gaggero, A. aut Gamborino, D. aut Garnier, P. aut Gibson, W. C. aut Goldstein, R. aut Grande, M. aut Grishin, V. aut Haggerty, D. aut Holmström, M. aut Horvath, I. aut Hsieh, K.-C. aut Jacques, A. aut Johnson, R. E. aut Kazakov, A. aut Kecskemety, K. aut Krüger, H. aut Kürbisch, C. aut Lazzarotto, F. aut Leblanc, Frederic aut Leichtfried, M. aut Leoni, R. aut Loose, A. aut Maschietti, D. aut Massetti, S. aut Mattioli, F. aut Miller, G. aut Moissenko, D. aut Morbidini, A. aut Noschese, R. aut Nuccilli, F. aut Nunez, C. aut Paschalidis, N. aut Persyn, S. aut Piazza, D. aut Oja, M. aut Ryno, J. aut Schmidt, W. aut Scheer, J. A. aut Shestakov, A. aut Shuvalov, S. aut Seki, K. aut Selci, S. aut Smith, K. aut Sordini, R. aut Svensson, J. aut Szalai, L. aut Toublanc, D. aut Urdiales, C. aut Varsani, A. aut Vertolli, N. aut Wallner, R. aut Wahlstroem, P. aut Wilson, P. aut Zampieri, S. aut Enthalten in Space science reviews Springer Netherlands, 1962 217(2021), 1 vom: 12. Jan. (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:217 year:2021 number:1 day:12 month:01 https://doi.org/10.1007/s11214-020-00787-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 AR 217 2021 1 12 01 |
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10.1007/s11214-020-00787-3 doi (DE-627)OLC2122641215 (DE-He213)s11214-020-00787-3-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Orsini, S. verfasserin aut SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021. corrected publication 2021 Abstract The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase. Mercury’s environment Particle instrumentation BepiColombo space mission Livi, S. A. aut Lichtenegger, H. aut Barabash, S. aut Milillo, A. aut De Angelis, E. aut Phillips, M. aut Laky, G. aut Wieser, M. aut Olivieri, A. aut Plainaki, C. aut Ho, G. aut Killen, R. M. aut Slavin, J. A. aut Wurz, P. aut Berthelier, J.-J. aut Dandouras, I. aut Kallio, E. aut McKenna-Lawlor, S. aut Szalai, S. aut Torkar, K. aut Vaisberg, O. aut Allegrini, F. aut Daglis, I. A. aut Dong, C. aut Escoubet, C. P. aut Fatemi, S. aut Fränz, M. aut Ivanovski, S. aut Krupp, N. aut Lammer, H. aut Leblanc, François aut Mangano, V. aut Mura, A. aut Nilsson, H. aut Raines, J. M. aut Rispoli, R. aut Sarantos, M. aut Smith, H. T. aut Szego, K. aut Aronica, A. aut Camozzi, F. aut Di Lellis, A. M. aut Fremuth, G. aut Giner, F. aut Gurnee, R. aut Hayes, J. aut Jeszenszky, H. aut Tominetti, F. aut Trantham, B. aut Balaz, J. aut Baumjohann, W. aut Brienza, D. aut Bührke, U. aut Bush, M. D. aut Cantatore, M. aut Cibella, S. aut Colasanti, L. aut Cremonese, G. aut Cremonesi, L. aut D’Alessandro, M. aut Delcourt, D. aut Delva, M. aut Desai, M. aut Fama, M. aut Ferris, M. aut Fischer, H. aut Gaggero, A. aut Gamborino, D. aut Garnier, P. aut Gibson, W. C. aut Goldstein, R. aut Grande, M. aut Grishin, V. aut Haggerty, D. aut Holmström, M. aut Horvath, I. aut Hsieh, K.-C. aut Jacques, A. aut Johnson, R. E. aut Kazakov, A. aut Kecskemety, K. aut Krüger, H. aut Kürbisch, C. aut Lazzarotto, F. aut Leblanc, Frederic aut Leichtfried, M. aut Leoni, R. aut Loose, A. aut Maschietti, D. aut Massetti, S. aut Mattioli, F. aut Miller, G. aut Moissenko, D. aut Morbidini, A. aut Noschese, R. aut Nuccilli, F. aut Nunez, C. aut Paschalidis, N. aut Persyn, S. aut Piazza, D. aut Oja, M. aut Ryno, J. aut Schmidt, W. aut Scheer, J. A. aut Shestakov, A. aut Shuvalov, S. aut Seki, K. aut Selci, S. aut Smith, K. aut Sordini, R. aut Svensson, J. aut Szalai, L. aut Toublanc, D. aut Urdiales, C. aut Varsani, A. aut Vertolli, N. aut Wallner, R. aut Wahlstroem, P. aut Wilson, P. aut Zampieri, S. aut Enthalten in Space science reviews Springer Netherlands, 1962 217(2021), 1 vom: 12. Jan. (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:217 year:2021 number:1 day:12 month:01 https://doi.org/10.1007/s11214-020-00787-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 AR 217 2021 1 12 01 |
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10.1007/s11214-020-00787-3 doi (DE-627)OLC2122641215 (DE-He213)s11214-020-00787-3-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Orsini, S. verfasserin aut SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021. corrected publication 2021 Abstract The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase. Mercury’s environment Particle instrumentation BepiColombo space mission Livi, S. A. aut Lichtenegger, H. aut Barabash, S. aut Milillo, A. aut De Angelis, E. aut Phillips, M. aut Laky, G. aut Wieser, M. aut Olivieri, A. aut Plainaki, C. aut Ho, G. aut Killen, R. M. aut Slavin, J. A. aut Wurz, P. aut Berthelier, J.-J. aut Dandouras, I. aut Kallio, E. aut McKenna-Lawlor, S. aut Szalai, S. aut Torkar, K. aut Vaisberg, O. aut Allegrini, F. aut Daglis, I. A. aut Dong, C. aut Escoubet, C. P. aut Fatemi, S. aut Fränz, M. aut Ivanovski, S. aut Krupp, N. aut Lammer, H. aut Leblanc, François aut Mangano, V. aut Mura, A. aut Nilsson, H. aut Raines, J. M. aut Rispoli, R. aut Sarantos, M. aut Smith, H. T. aut Szego, K. aut Aronica, A. aut Camozzi, F. aut Di Lellis, A. M. aut Fremuth, G. aut Giner, F. aut Gurnee, R. aut Hayes, J. aut Jeszenszky, H. aut Tominetti, F. aut Trantham, B. aut Balaz, J. aut Baumjohann, W. aut Brienza, D. aut Bührke, U. aut Bush, M. D. aut Cantatore, M. aut Cibella, S. aut Colasanti, L. aut Cremonese, G. aut Cremonesi, L. aut D’Alessandro, M. aut Delcourt, D. aut Delva, M. aut Desai, M. aut Fama, M. aut Ferris, M. aut Fischer, H. aut Gaggero, A. aut Gamborino, D. aut Garnier, P. aut Gibson, W. C. aut Goldstein, R. aut Grande, M. aut Grishin, V. aut Haggerty, D. aut Holmström, M. aut Horvath, I. aut Hsieh, K.-C. aut Jacques, A. aut Johnson, R. E. aut Kazakov, A. aut Kecskemety, K. aut Krüger, H. aut Kürbisch, C. aut Lazzarotto, F. aut Leblanc, Frederic aut Leichtfried, M. aut Leoni, R. aut Loose, A. aut Maschietti, D. aut Massetti, S. aut Mattioli, F. aut Miller, G. aut Moissenko, D. aut Morbidini, A. aut Noschese, R. aut Nuccilli, F. aut Nunez, C. aut Paschalidis, N. aut Persyn, S. aut Piazza, D. aut Oja, M. aut Ryno, J. aut Schmidt, W. aut Scheer, J. A. aut Shestakov, A. aut Shuvalov, S. aut Seki, K. aut Selci, S. aut Smith, K. aut Sordini, R. aut Svensson, J. aut Szalai, L. aut Toublanc, D. aut Urdiales, C. aut Varsani, A. aut Vertolli, N. aut Wallner, R. aut Wahlstroem, P. aut Wilson, P. aut Zampieri, S. aut Enthalten in Space science reviews Springer Netherlands, 1962 217(2021), 1 vom: 12. Jan. (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:217 year:2021 number:1 day:12 month:01 https://doi.org/10.1007/s11214-020-00787-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 AR 217 2021 1 12 01 |
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10.1007/s11214-020-00787-3 doi (DE-627)OLC2122641215 (DE-He213)s11214-020-00787-3-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Orsini, S. verfasserin aut SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021. corrected publication 2021 Abstract The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase. Mercury’s environment Particle instrumentation BepiColombo space mission Livi, S. A. aut Lichtenegger, H. aut Barabash, S. aut Milillo, A. aut De Angelis, E. aut Phillips, M. aut Laky, G. aut Wieser, M. aut Olivieri, A. aut Plainaki, C. aut Ho, G. aut Killen, R. M. aut Slavin, J. A. aut Wurz, P. aut Berthelier, J.-J. aut Dandouras, I. aut Kallio, E. aut McKenna-Lawlor, S. aut Szalai, S. aut Torkar, K. aut Vaisberg, O. aut Allegrini, F. aut Daglis, I. A. aut Dong, C. aut Escoubet, C. P. aut Fatemi, S. aut Fränz, M. aut Ivanovski, S. aut Krupp, N. aut Lammer, H. aut Leblanc, François aut Mangano, V. aut Mura, A. aut Nilsson, H. aut Raines, J. M. aut Rispoli, R. aut Sarantos, M. aut Smith, H. T. aut Szego, K. aut Aronica, A. aut Camozzi, F. aut Di Lellis, A. M. aut Fremuth, G. aut Giner, F. aut Gurnee, R. aut Hayes, J. aut Jeszenszky, H. aut Tominetti, F. aut Trantham, B. aut Balaz, J. aut Baumjohann, W. aut Brienza, D. aut Bührke, U. aut Bush, M. D. aut Cantatore, M. aut Cibella, S. aut Colasanti, L. aut Cremonese, G. aut Cremonesi, L. aut D’Alessandro, M. aut Delcourt, D. aut Delva, M. aut Desai, M. aut Fama, M. aut Ferris, M. aut Fischer, H. aut Gaggero, A. aut Gamborino, D. aut Garnier, P. aut Gibson, W. C. aut Goldstein, R. aut Grande, M. aut Grishin, V. aut Haggerty, D. aut Holmström, M. aut Horvath, I. aut Hsieh, K.-C. aut Jacques, A. aut Johnson, R. E. aut Kazakov, A. aut Kecskemety, K. aut Krüger, H. aut Kürbisch, C. aut Lazzarotto, F. aut Leblanc, Frederic aut Leichtfried, M. aut Leoni, R. aut Loose, A. aut Maschietti, D. aut Massetti, S. aut Mattioli, F. aut Miller, G. aut Moissenko, D. aut Morbidini, A. aut Noschese, R. aut Nuccilli, F. aut Nunez, C. aut Paschalidis, N. aut Persyn, S. aut Piazza, D. aut Oja, M. aut Ryno, J. aut Schmidt, W. aut Scheer, J. A. aut Shestakov, A. aut Shuvalov, S. aut Seki, K. aut Selci, S. aut Smith, K. aut Sordini, R. aut Svensson, J. aut Szalai, L. aut Toublanc, D. aut Urdiales, C. aut Varsani, A. aut Vertolli, N. aut Wallner, R. aut Wahlstroem, P. aut Wilson, P. aut Zampieri, S. aut Enthalten in Space science reviews Springer Netherlands, 1962 217(2021), 1 vom: 12. Jan. (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:217 year:2021 number:1 day:12 month:01 https://doi.org/10.1007/s11214-020-00787-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 AR 217 2021 1 12 01 |
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10.1007/s11214-020-00787-3 doi (DE-627)OLC2122641215 (DE-He213)s11214-020-00787-3-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Orsini, S. verfasserin aut SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021. corrected publication 2021 Abstract The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase. Mercury’s environment Particle instrumentation BepiColombo space mission Livi, S. A. aut Lichtenegger, H. aut Barabash, S. aut Milillo, A. aut De Angelis, E. aut Phillips, M. aut Laky, G. aut Wieser, M. aut Olivieri, A. aut Plainaki, C. aut Ho, G. aut Killen, R. M. aut Slavin, J. A. aut Wurz, P. aut Berthelier, J.-J. aut Dandouras, I. aut Kallio, E. aut McKenna-Lawlor, S. aut Szalai, S. aut Torkar, K. aut Vaisberg, O. aut Allegrini, F. aut Daglis, I. A. aut Dong, C. aut Escoubet, C. P. aut Fatemi, S. aut Fränz, M. aut Ivanovski, S. aut Krupp, N. aut Lammer, H. aut Leblanc, François aut Mangano, V. aut Mura, A. aut Nilsson, H. aut Raines, J. M. aut Rispoli, R. aut Sarantos, M. aut Smith, H. T. aut Szego, K. aut Aronica, A. aut Camozzi, F. aut Di Lellis, A. M. aut Fremuth, G. aut Giner, F. aut Gurnee, R. aut Hayes, J. aut Jeszenszky, H. aut Tominetti, F. aut Trantham, B. aut Balaz, J. aut Baumjohann, W. aut Brienza, D. aut Bührke, U. aut Bush, M. D. aut Cantatore, M. aut Cibella, S. aut Colasanti, L. aut Cremonese, G. aut Cremonesi, L. aut D’Alessandro, M. aut Delcourt, D. aut Delva, M. aut Desai, M. aut Fama, M. aut Ferris, M. aut Fischer, H. aut Gaggero, A. aut Gamborino, D. aut Garnier, P. aut Gibson, W. C. aut Goldstein, R. aut Grande, M. aut Grishin, V. aut Haggerty, D. aut Holmström, M. aut Horvath, I. aut Hsieh, K.-C. aut Jacques, A. aut Johnson, R. E. aut Kazakov, A. aut Kecskemety, K. aut Krüger, H. aut Kürbisch, C. aut Lazzarotto, F. aut Leblanc, Frederic aut Leichtfried, M. aut Leoni, R. aut Loose, A. aut Maschietti, D. aut Massetti, S. aut Mattioli, F. aut Miller, G. aut Moissenko, D. aut Morbidini, A. aut Noschese, R. aut Nuccilli, F. aut Nunez, C. aut Paschalidis, N. aut Persyn, S. aut Piazza, D. aut Oja, M. aut Ryno, J. aut Schmidt, W. aut Scheer, J. A. aut Shestakov, A. aut Shuvalov, S. aut Seki, K. aut Selci, S. aut Smith, K. aut Sordini, R. aut Svensson, J. aut Szalai, L. aut Toublanc, D. aut Urdiales, C. aut Varsani, A. aut Vertolli, N. aut Wallner, R. aut Wahlstroem, P. aut Wilson, P. aut Zampieri, S. aut Enthalten in Space science reviews Springer Netherlands, 1962 217(2021), 1 vom: 12. Jan. (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:217 year:2021 number:1 day:12 month:01 https://doi.org/10.1007/s11214-020-00787-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 AR 217 2021 1 12 01 |
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The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. 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Orsini, S. Livi, S. A. Lichtenegger, H. Barabash, S. Milillo, A. De Angelis, E. Phillips, M. Laky, G. Wieser, M. Olivieri, A. Plainaki, C. Ho, G. Killen, R. M. Slavin, J. A. Wurz, P. Berthelier, J.-J. Dandouras, I. Kallio, E. McKenna-Lawlor, S. Szalai, S. Torkar, K. Vaisberg, O. Allegrini, F. Daglis, I. A. Dong, C. Escoubet, C. P. Fatemi, S. Fränz, M. Ivanovski, S. Krupp, N. Lammer, H. Leblanc, François Mangano, V. Mura, A. Nilsson, H. Raines, J. M. Rispoli, R. Sarantos, M. Smith, H. T. Szego, K. Aronica, A. Camozzi, F. Di Lellis, A. M. Fremuth, G. Giner, F. Gurnee, R. Hayes, J. Jeszenszky, H. Tominetti, F. Trantham, B. Balaz, J. Baumjohann, W. Brienza, D. Bührke, U. Bush, M. D. Cantatore, M. Cibella, S. Colasanti, L. Cremonese, G. Cremonesi, L. D’Alessandro, M. Delcourt, D. Delva, M. Desai, M. Fama, M. Ferris, M. Fischer, H. Gaggero, A. Gamborino, D. Garnier, P. Gibson, W. C. Goldstein, R. Grande, M. Grishin, V. Haggerty, D. Holmström, M. Horvath, I. Hsieh, K.-C. Jacques, A. Johnson, R. E. Kazakov, A. Kecskemety, K. Krüger, H. Kürbisch, C. Lazzarotto, F. Leblanc, Frederic Leichtfried, M. Leoni, R. Loose, A. Maschietti, D. Massetti, S. Mattioli, F. Miller, G. Moissenko, D. Morbidini, A. Noschese, R. Nuccilli, F. Nunez, C. Paschalidis, N. Persyn, S. Piazza, D. Oja, M. Ryno, J. Schmidt, W. Scheer, J. A. Shestakov, A. Shuvalov, S. Seki, K. Selci, S. Smith, K. Sordini, R. Svensson, J. Szalai, L. Toublanc, D. Urdiales, C. Varsani, A. Vertolli, N. Wallner, R. Wahlstroem, P. Wilson, P. Zampieri, S. |
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serena: particle instrument suite for determining the sun-mercury interaction from bepicolombo |
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SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo |
abstract |
Abstract The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase. © The Author(s) 2021. corrected publication 2021 |
abstractGer |
Abstract The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase. © The Author(s) 2021. corrected publication 2021 |
abstract_unstemmed |
Abstract The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase. © The Author(s) 2021. corrected publication 2021 |
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title_short |
SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo |
url |
https://doi.org/10.1007/s11214-020-00787-3 |
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author2 |
Livi, S. A. Lichtenegger, H. Barabash, S. Milillo, A. De Angelis, E. Phillips, M. Laky, G. Wieser, M. Olivieri, A. Plainaki, C. Ho, G. Killen, R. M. Slavin, J. A. Wurz, P. Berthelier, J.-J. Dandouras, I. Kallio, E. McKenna-Lawlor, S. Szalai, S. Torkar, K. Vaisberg, O. Allegrini, F. Daglis, I. A. Dong, C. Escoubet, C. P. Fatemi, S. Fränz, M. Ivanovski, S. Krupp, N. Lammer, H. Leblanc, François Mangano, V. Mura, A. Nilsson, H. Raines, J. M. Rispoli, R. Sarantos, M. Smith, H. T. Szego, K. Aronica, A. Camozzi, F. Di Lellis, A. M. Fremuth, G. Giner, F. Gurnee, R. Hayes, J. Jeszenszky, H. Tominetti, F. Trantham, B. Balaz, J. Baumjohann, W. Brienza, D. Bührke, U. Bush, M. D. Cantatore, M. Cibella, S. Colasanti, L. Cremonese, G. Cremonesi, L. D’Alessandro, M. Delcourt, D. Delva, M. Desai, M. Fama, M. Ferris, M. Fischer, H. Gaggero, A. Gamborino, D. Garnier, P. Gibson, W. C. Goldstein, R. Grande, M. Grishin, V. Haggerty, D. Holmström, M. Horvath, I. Hsieh, K.-C. Jacques, A. Johnson, R. E. Kazakov, A. Kecskemety, K. Krüger, H. Kürbisch, C. Lazzarotto, F. Leblanc, Frederic Leichtfried, M. Leoni, R. Loose, A. Maschietti, D. Massetti, S. Mattioli, F. Miller, G. Moissenko, D. Morbidini, A. Noschese, R. Nuccilli, F. Nunez, C. Paschalidis, N. Persyn, S. Piazza, D. Oja, M. Ryno, J. Schmidt, W. Scheer, J. A. Shestakov, A. Shuvalov, S. Seki, K. Selci, S. Smith, K. Sordini, R. Svensson, J. Szalai, L. Toublanc, D. Urdiales, C. Varsani, A. Vertolli, N. Wallner, R. Wahlstroem, P. Wilson, P. Zampieri, S. |
author2Str |
Livi, S. A. Lichtenegger, H. Barabash, S. Milillo, A. De Angelis, E. Phillips, M. Laky, G. Wieser, M. Olivieri, A. Plainaki, C. Ho, G. Killen, R. M. Slavin, J. A. Wurz, P. Berthelier, J.-J. Dandouras, I. Kallio, E. McKenna-Lawlor, S. Szalai, S. Torkar, K. Vaisberg, O. Allegrini, F. Daglis, I. A. Dong, C. Escoubet, C. P. Fatemi, S. Fränz, M. Ivanovski, S. Krupp, N. Lammer, H. Leblanc, François Mangano, V. Mura, A. Nilsson, H. Raines, J. M. Rispoli, R. Sarantos, M. Smith, H. T. Szego, K. Aronica, A. Camozzi, F. Di Lellis, A. M. Fremuth, G. Giner, F. Gurnee, R. Hayes, J. Jeszenszky, H. Tominetti, F. Trantham, B. Balaz, J. Baumjohann, W. Brienza, D. Bührke, U. Bush, M. D. Cantatore, M. Cibella, S. Colasanti, L. Cremonese, G. Cremonesi, L. D’Alessandro, M. Delcourt, D. Delva, M. Desai, M. Fama, M. Ferris, M. Fischer, H. Gaggero, A. Gamborino, D. Garnier, P. Gibson, W. C. Goldstein, R. Grande, M. Grishin, V. Haggerty, D. Holmström, M. Horvath, I. Hsieh, K.-C. Jacques, A. Johnson, R. E. Kazakov, A. Kecskemety, K. Krüger, H. Kürbisch, C. Lazzarotto, F. Leblanc, Frederic Leichtfried, M. Leoni, R. Loose, A. Maschietti, D. Massetti, S. Mattioli, F. Miller, G. Moissenko, D. Morbidini, A. Noschese, R. Nuccilli, F. Nunez, C. Paschalidis, N. Persyn, S. Piazza, D. Oja, M. Ryno, J. Schmidt, W. Scheer, J. A. Shestakov, A. Shuvalov, S. Seki, K. Selci, S. Smith, K. Sordini, R. Svensson, J. Szalai, L. Toublanc, D. Urdiales, C. Varsani, A. Vertolli, N. Wallner, R. Wahlstroem, P. Wilson, P. Zampieri, S. |
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