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
Hauptverfasser: 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.
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container_title Astronomy and astrophysics (Berlin)
container_volume 642
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
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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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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. 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R.</au><au>Whiteside, B.</au><au>Bale, S. D.</au><au>Baumjohann, W.</au><au>Burgess, D.</au><au>Carbone, V.</au><au>Cargill, P.</au><au>Eastwood, J.</au><au>Erdös, G.</au><au>Fletcher, L.</au><au>Forsyth, R.</au><au>Giacalone, J.</au><au>Glassmeier, K.-H.</au><au>Goldstein, M. L.</au><au>Hoeksema, T.</au><au>Lockwood, M.</au><au>Magnes, W.</au><au>Maksimovic, M.</au><au>Marsch, E.</au><au>Matthaeus, W. H.</au><au>Murphy, N.</au><au>Nakariakov, V. M.</au><au>Owen, C. J.</au><au>Owens, M.</au><au>Rodriguez-Pacheco, J.</au><au>Richter, I.</au><au>Riley, P.</au><au>Russell, C. T.</au><au>Schwartz, S.</au><au>Vainio, R.</au><au>Velli, M.</au><au>Vennerstrom, S.</au><au>Walsh, R.</au><au>Wimmer-Schweingruber, R. F.</au><au>Zank, G.</au><au>Müller, D.</au><au>Zouganelis, I.</au><au>Walsh, A. P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Solar Orbiter magnetometer</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2020-10-01</date><risdate>2020</risdate><volume>642</volume><spage>A9</spage><pages>A9-</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><eissn>1432-0756</eissn><abstract>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.</abstract><cop>Heidelberg</cop><pub>EDP Sciences</pub><doi>10.1051/0004-6361/201937257</doi><orcidid>https://orcid.org/0000-0002-1989-3596</orcidid><orcidid>https://orcid.org/0000-0001-6271-0110</orcidid><orcidid>https://orcid.org/0000-0003-3732-137X</orcidid><orcidid>https://orcid.org/0000-0002-6879-3970</orcidid><orcidid>https://orcid.org/0000-0001-7224-6024</orcidid><orcidid>https://orcid.org/0000-0002-1152-1114</orcidid><orcidid>https://orcid.org/0000-0003-0086-6288</orcidid><orcidid>https://orcid.org/0000-0003-4733-8319</orcidid><orcidid>https://orcid.org/0000-0003-1639-8298</orcidid><orcidid>https://orcid.org/0000-0001-5834-9588</orcidid><orcidid>https://orcid.org/0000-0001-6172-5062</orcidid><orcidid>https://orcid.org/0000-0001-5475-9379</orcidid><orcidid>https://orcid.org/0000-0002-2381-3106</orcidid><orcidid>https://orcid.org/0000-0002-5982-4667</orcidid><oa>free_for_read</oa></addata></record>
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identifier ISSN: 0004-6361
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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