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The Solar Orbiter Science Activity Plan: Translating solar and heliospheric physics questions into action

  • I. Zouganelis
  • , A. De Groof
  • , A. P. Walsh
  • , D. R. Williams
  • , D. Müller
  • , O. C. St Cyr
  • , F. Auchère
  • , D. Berghmans
  • , A. Fludra
  • , T. S. Horbury
  • , R. A. Howard
  • , S. Krucker
  • , M. Maksimovic
  • , C. J. Owen
  • , J. Rodríguez-Pacheco
  • , M. Romoli
  • , S. K. Solanki
  • , C. Watson
  • , L. Sanchez
  • , J. Lefort
  • P. Osuna, H. R. Gilbert, T. Nieves-Chinchilla, L. Abbo, O. Alexandrova, A. Anastasiadis, V. Andretta, E. Antonucci, T. Appourchaux, A. Aran, C. N. Arge, G. Aulanier, D. Baker, S. D. Bale, M. Battaglia, L. Bellot Rubio, A. Bemporad, M. Berthomier, K. Bocchialini, X. Bonnin, A. S. Brun, R. Bruno, E. Buchlin, J. Büchner, R. Bucik, F. Carcaboso, R. Carr, I. Carrasco-Blázquez, B. Cecconi, I. Cernuda Cangas, C. H.K. Chen, L. P. Chitta, T. Chust, K. Dalmasse, R. D'Amicis, V. Da Deppo, R. De Marco, S. Dolei, L. Dolla, T. Dudok De Wit, L. Van Driel-Gesztelyi, J. P. Eastwood, F. Espinosa Lara, L. Etesi, A. Fedorov, F. Félix-Redondo, S. Fineschi, B. Fleck, D. Fontaine, N. J. Fox, A. Gandorfer, V. Génot, M. K. Georgoulis, S. Gissot, A. Giunta, L. Gizon, R. Gómez-Herrero, C. Gontikakis, G. Graham, L. Green, T. Grundy, M. Haberreiter, L. K. Harra, D. M. Hassler, J. Hirzberger, G. C. Ho, G. Hurford, D. Innes, K. Issautier, A. W. James, N. Janitzek, M. Janvier, N. Jeffrey, J. Jenkins, Y. Khotyaintsev, K. L. Klein, E. P. Kontar, I. Kontogiannis, C. Krafft, V. Krasnoselskikh, M. Kretzschmar, N. Labrosse, A. Lagg, F. Landini, B. Lavraud, I. Leon, S. T. Lepri, G. R. Lewis, P. Liewer, J. Linker, S. Livi, D. M. Long, P. Louarn, O. Malandraki, S. Maloney, V. Martinez-Pillet, M. Martinovic, A. Masson, S. Matthews, L. Matteini, N. Meyer-Vernet, K. Moraitis, R. J. Morton, S. Musset, G. Nicolaou, A. Nindos, H. O'Brien, D. Orozco Suarez, M. Owens, M. Pancrazzi, A. Papaioannou, S. Parenti, E. Pariat, S. Patsourakos, D. Perrone, H. Peter, R. F. Pinto, C. Plainaki, D. Plettemeier, S. P. Plunkett, J. M. Raines, N. Raouafi, H. Reid, A. Retino, L. Rezeau, P. Rochus, L. Rodriguez, L. Rodriguez-Garcia, M. Roth, A. P. Rouillard, F. Sahraoui, C. Sasso, J. Schou, U. Schühle, L. Sorriso-Valvo, J. Soucek, D. Spadaro, M. Stangalini, D. Stansby, M. Steller, A. Strugarek, Štverák, R. Susino, D. Telloni, C. Terasa, L. Teriaca, S. Toledo-Redondo, J. C. Del Toro Iniesta, G. Tsiropoula, A. Tsounis, K. Tziotziou, F. Valentini, A. Vaivads, A. Vecchio, M. Velli, C. Verbeeck, A. Verdini, D. Verscharen, N. Vilmer, A. Vourlidas, R. Wicks, R. F. Wimmer-Schweingruber, T. Wiegelmann, P. R. Young, A. N. Zhukov
  • European Space Agency - ESA
  • ESTEC
  • NASA Goddard Space Flight Center
  • Université Paris-Saclay
  • Royal Observatory of Belgium
  • Rutherford Appleton Laboratory
  • Imperial College London
  • Naval Research Laboratory
  • University of Applied Sciences Northwestern Switzerland
  • Observatoire de Paris
  • University College London
  • University of Alcalá
  • University of Florence
  • Max Planck Institute for Solar System Research
  • Kyung Hee University
  • National Institute for Astrophysics
  • National Observatory of Athens
  • Osservatorio Astronomico di Capodimonte
  • University of Barcelona
  • University of California at Berkeley
  • CSIC - Institute of Astrophysics of Andalusia
  • Sorbonne Université
  • Technical University of Berlin
  • Southwest Research Institute
  • Queen Mary University of London
  • Université de Toulouse
  • National Research Council of Italy
  • Osservatorio Astrofisico di Catania
  • Université d'Orléans
  • National Aeronautics and Space Administration
  • Academy of Athens
  • Georgia State University
  • Physikalisch-Meteorologisches Observatorium Davos World Radiation Center
  • Swiss Federal Institute of Technology Zurich
  • Johns Hopkins University Applied Physics Laboratory
  • Northumbria University
  • KU Leuven
  • Swedish Institute of Space Physics
  • University of Glasgow
  • Leibniz Institute for Astrophysics Potsdam
  • University of Michigan, Ann Arbor
  • Jet Propulsion Laboratory, California Institute of Technology
  • Predictive Science Inc
  • Trinity College Dublin
  • Dublin Institute for Advanced Studies
  • National Solar Observatory
  • University of Arizona
  • University of Ioannina
  • University of Reading
  • Osservatorio Astrofisico Di Arcetri, Florence
  • Italian Space Agency
  • Technische Universität Dresden
  • University of Liege
  • Leibniz-Institut fuer Sonnenphysik (KIS)
  • Escuela Politécnica Nacional
  • Czech Academy of Sciences
  • Austrian Academy of Sciences
  • Kiel University
  • University of Murcia
  • University of Calabria
  • KTH Royal Institute of Technology
  • Radboud University Nijmegen
  • University of New Hampshire
  • Lomonosov Moscow State University

Research output: Contribution to journalArticlepeer-review

102 Scopus citations

Abstract

Solar Orbiter is the first space mission observing the solar plasma both in situ and remotely, from a close distance, in and out of the ecliptic. The ultimate goal is to understand how the Sun produces and controls the heliosphere, filling the Solar System and driving the planetary environments. With six remote-sensing and four in-situ instrument suites, the coordination and planning of the operations are essential to address the following four top-level science questions: (1) What drives the solar wind and where does the coronal magnetic field originate?; (2) How do solar transients drive heliospheric variability?; (3) How do solar eruptions produce energetic particle radiation that fills the heliosphere?; (4) How does the solar dynamo work and drive connections between the Sun and the heliosphere? Maximising the mission's science return requires considering the characteristics of each orbit, including the relative position of the spacecraft to Earth (affecting downlink rates), trajectory events (such as gravitational assist manoeuvres), and the phase of the solar activity cycle. Furthermore, since each orbit's science telemetry will be downloaded over the course of the following orbit, science operations must be planned at mission level, rather than at the level of individual orbits. It is important to explore the way in which those science questions are translated into an actual plan of observations that fits into the mission, thus ensuring that no opportunities are missed. First, the overarching goals are broken down into specific, answerable questions along with the required observations and the so-called Science Activity Plan (SAP) is developed to achieve this. The SAP groups objectives that require similar observations into Solar Orbiter Observing Plans, resulting in a strategic, top-level view of the optimal opportunities for science observations during the mission lifetime. This allows for all four mission goals to be addressed. In this paper, we introduce Solar Orbiter's SAP through a series of examples and the strategy being followed.

Original languageEnglish
Article numberA3
JournalAstronomy and Astrophysics
Volume642
DOIs
StatePublished - Oct 1 2020
Externally publishedYes

Keywords

  • Methods: observational
  • Space vehicles: instruments
  • Sun: general

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