The Solar Orbiter magnetometer
The magnetometer instrument on the Solar Orbiter mission is designed to measure the magnetic field local to the spacecraft continuously for the entire mission duration. The need to characterise not only the background magnetic field but also its variations on scales from far above to well below the...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2020-10, Vol.642, p.A9 |
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creator | Horbury, T. S. O’Brien, H. Carrasco Blazquez, I. Bendyk, M. Brown, P. Hudson, R. Evans, V. Oddy, T. M. Carr, C. M. Beek, T. J. Cupido, E. Bhattacharya, S. Dominguez, J.-A. Matthews, L. Myklebust, V. R. Whiteside, B. Bale, S. D. Baumjohann, W. Burgess, D. Carbone, V. Cargill, P. Eastwood, J. Erdös, G. Fletcher, L. Forsyth, R. Giacalone, J. Glassmeier, K.-H. Goldstein, M. L. Hoeksema, T. Lockwood, M. Magnes, W. Maksimovic, M. Marsch, E. Matthaeus, W. H. Murphy, N. Nakariakov, V. M. Owen, C. J. Owens, M. Rodriguez-Pacheco, J. Richter, I. Riley, P. Russell, C. T. Schwartz, S. Vainio, R. Velli, M. Vennerstrom, S. Walsh, R. Wimmer-Schweingruber, R. F. Zank, G. Müller, D. Zouganelis, I. Walsh, A. P. |
description | The magnetometer instrument on the Solar Orbiter mission is designed to measure the magnetic field local to the spacecraft continuously for the entire mission duration. The need to characterise not only the background magnetic field but also its variations on scales from far above to well below the proton gyroscale result in challenging requirements on stability, precision, and noise, as well as magnetic and operational limitations on both the spacecraft and other instruments. The challenging vibration and thermal environment has led to significant development of the mechanical sensor design. The overall instrument design, performance, data products, and operational strategy are described. |
doi_str_mv | 10.1051/0004-6361/201937257 |
format | Article |
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S. ; O’Brien, H. ; Carrasco Blazquez, I. ; Bendyk, M. ; Brown, P. ; Hudson, R. ; Evans, V. ; Oddy, T. M. ; Carr, C. M. ; Beek, T. J. ; Cupido, E. ; Bhattacharya, S. ; Dominguez, J.-A. ; Matthews, L. ; Myklebust, V. R. ; Whiteside, B. ; Bale, S. D. ; Baumjohann, W. ; Burgess, D. ; Carbone, V. ; Cargill, P. ; Eastwood, J. ; Erdös, G. ; Fletcher, L. ; Forsyth, R. ; Giacalone, J. ; Glassmeier, K.-H. ; Goldstein, M. L. ; Hoeksema, T. ; Lockwood, M. ; Magnes, W. ; Maksimovic, M. ; Marsch, E. ; Matthaeus, W. H. ; Murphy, N. ; Nakariakov, V. M. ; Owen, C. J. ; Owens, M. ; Rodriguez-Pacheco, J. ; Richter, I. ; Riley, P. ; Russell, C. T. ; Schwartz, S. ; Vainio, R. ; Velli, M. ; Vennerstrom, S. ; Walsh, R. ; Wimmer-Schweingruber, R. F. ; Zank, G. ; Müller, D. ; Zouganelis, I. ; Walsh, A. P.</creator><creatorcontrib>Horbury, T. S. ; O’Brien, H. ; Carrasco Blazquez, I. ; Bendyk, M. ; Brown, P. ; Hudson, R. ; Evans, V. ; Oddy, T. M. ; Carr, C. M. ; Beek, T. 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S.</creatorcontrib><creatorcontrib>O’Brien, H.</creatorcontrib><creatorcontrib>Carrasco Blazquez, I.</creatorcontrib><creatorcontrib>Bendyk, M.</creatorcontrib><creatorcontrib>Brown, P.</creatorcontrib><creatorcontrib>Hudson, R.</creatorcontrib><creatorcontrib>Evans, V.</creatorcontrib><creatorcontrib>Oddy, T. M.</creatorcontrib><creatorcontrib>Carr, C. M.</creatorcontrib><creatorcontrib>Beek, T. J.</creatorcontrib><creatorcontrib>Cupido, E.</creatorcontrib><creatorcontrib>Bhattacharya, S.</creatorcontrib><creatorcontrib>Dominguez, J.-A.</creatorcontrib><creatorcontrib>Matthews, L.</creatorcontrib><creatorcontrib>Myklebust, V. R.</creatorcontrib><creatorcontrib>Whiteside, B.</creatorcontrib><creatorcontrib>Bale, S. 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J.</creatorcontrib><creatorcontrib>Owens, M.</creatorcontrib><creatorcontrib>Rodriguez-Pacheco, J.</creatorcontrib><creatorcontrib>Richter, I.</creatorcontrib><creatorcontrib>Riley, P.</creatorcontrib><creatorcontrib>Russell, C. T.</creatorcontrib><creatorcontrib>Schwartz, S.</creatorcontrib><creatorcontrib>Vainio, R.</creatorcontrib><creatorcontrib>Velli, M.</creatorcontrib><creatorcontrib>Vennerstrom, S.</creatorcontrib><creatorcontrib>Walsh, R.</creatorcontrib><creatorcontrib>Wimmer-Schweingruber, R. F.</creatorcontrib><creatorcontrib>Zank, G.</creatorcontrib><creatorcontrib>Müller, D.</creatorcontrib><creatorcontrib>Zouganelis, I.</creatorcontrib><creatorcontrib>Walsh, A. P.</creatorcontrib><title>The Solar Orbiter magnetometer</title><title>Astronomy and astrophysics (Berlin)</title><description>The magnetometer instrument on the Solar Orbiter mission is designed to measure the magnetic field local to the spacecraft continuously for the entire mission duration. 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ispartof | Astronomy and astrophysics (Berlin), 2020-10, Vol.642, p.A9 |
issn | 0004-6361 1432-0746 1432-0756 |
language | eng |
recordid | cdi_hal_primary_oai_HAL_hal_03256356v1 |
source | Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; EDP Sciences; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals |
subjects | Astrophysics Magnetic fields Magnetometers Physics Spacecraft Thermal environments |
title | The Solar Orbiter magnetometer |
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