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 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.

[1]  P. Kletzkine,et al.  Solar Orbiter: Mission and spacecraft design , 2020, Astronomy & Astrophysics.

[2]  A. M. Hellín,et al.  The Energetic Particle Detector , 2020 .

[3]  X. Bonnin,et al.  Coordination of the in situ payload of Solar Orbiter , 2020, Astronomy & Astrophysics.

[4]  N. Raouafi,et al.  Understanding the origins of the heliosphere: integrating observations and measurements from Parker Solar Probe, Solar Orbiter, and other space- and ground-based observatories , 2020, Astronomy & Astrophysics.

[5]  P. Astier,et al.  The Solar Orbiter Radio and Plasma Waves (RPW) instrument , 2020, Astronomy & Astrophysics.

[6]  D. Plettemeier,et al.  The Solar Orbiter Science Activity Plan , 2020, Astronomy & Astrophysics.

[7]  A. Spencer,et al.  The Solar Orbiter Solar Wind Analyser (SWA) suite , 2020, Astronomy & Astrophysics.

[8]  J. C. del Toro Iniesta,et al.  The Polarimetric and Helioseismic Imager on Solar Orbiter , 2019, Astronomy & Astrophysics.

[9]  D. Stansby,et al.  Highly structured slow solar wind emerging from an equatorial coronal hole , 2019, Nature.

[10]  N. Pogorelov,et al.  Alfvénic velocity spikes and rotational flows in the near-Sun solar wind , 2019, Nature.

[11]  L. Matteini,et al.  On slow solar wind with high Alfvénicity: from composition and microphysics to spectral properties , 2018, Monthly Notices of the Royal Astronomical Society.

[12]  G. Vichare,et al.  The Identification of a Planar Magnetic Structure within the ICME Shock Sheath and Its influence on Galactic Cosmic-Ray Flux , 2018, The Astrophysical Journal.

[13]  T. Horbury,et al.  Short, large-amplitude speed enhancements in the near-Sunfast solar wind , 2018 .

[14]  Y.-M. Wang Small Coronal Holes Near Active Regions as Sources of Slow Solar Wind , 2017 .

[15]  M. Lockwood,et al.  The Solar Probe Plus Mission: Humanity’s First Visit to Our Star , 2016 .

[16]  Gernot Kubin,et al.  Optimized Merging of Search Coil and Fluxgate Data for MMS , 2016 .

[17]  A. Schekochihin,et al.  MULTI-SPECIES MEASUREMENTS OF THE FIREHOSE AND MIRROR INSTABILITY THRESHOLDS IN THE SOLAR WIND , 2016, 1606.02624.

[18]  J. C. del Toro Iniesta,et al.  The Solar Orbiter mission , 2020, Optics & Photonics - Optical Engineering + Applications.

[19]  D. Müller,et al.  Solar Orbiter , 2012, Solar Physics.

[20]  X. Dou,et al.  Geomagnetic and auroral activity driven by corotating interaction regions during the declining phase of Solar Cycle 23 , 2012 .

[21]  N. Sheeley,et al.  ON THE NATURE OF THE SOLAR WIND FROM CORONAL PSEUDOSTREAMERS , 2012 .

[22]  D. Müller,et al.  Solar Orbiter , 2012, Solar Physics.

[23]  N. Sheeley,et al.  ON THE WEAKENING OF THE POLAR MAGNETIC FIELDS DURING SOLAR CYCLE 23 , 2009 .

[24]  J. Eastwood The science of space weather , 2008, Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences.

[25]  E. Cupido,et al.  A radiation tolerant digital fluxgate magnetometer , 2007 .

[26]  Petr Hellinger,et al.  Evolution of the solar wind proton temperature anisotropy from 0.3 to 2.5 AU , 2007 .

[27]  K. Glassmeier,et al.  RPC-MAG The Fluxgate Magnetometer in the ROSETTA Plasma Consortium , 2007 .

[28]  Werner Magnes,et al.  The Double Star magnetic field investigation: instrument design, performance and highlights of the first year's observations , 2005 .

[29]  K.-H. Glassmeier,et al.  The Cassini Magnetic Field Investigation , 2004 .

[30]  J. Geiss,et al.  The Sun and Heliosphere at Solar Maximum , 2003, Science.

[31]  Mario H. Acuna,et al.  Space-based magnetometers , 2002 .

[32]  S. Cranmer Coronal Holes and the High-Speed Solar Wind , 2002 .

[33]  A. Balogh,et al.  Context and heliographic dependence of heliospheric planar magnetic structures , 2000 .

[34]  R. Kallenbach,et al.  Corotating Interaction Regions , 1999 .

[35]  Eckart Marsch,et al.  Physics of the Inner Heliosphere II , 1990 .

[36]  Eckart Marsch,et al.  Physics of the Inner Heliosphere I. Large-Scale Phenomena. , 1990 .

[37]  E. Hogenauer,et al.  An economical class of digital filters for decimation and interpolation , 1981 .

[38]  K. Schatten,et al.  Theoretical and observational analysis of spacecraft fields , 1974 .