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The Solar Orbiter Science Activity Plan

112Citations signalées, ce qui n’est pas une note de qualité
83Institutions déclarées
17Pays d’affiliation déclarés

Rattachement africain : es, nl, us, fr, be, gb, ch, it, kr, de, gr, se, ie, ec, cz, at, ru. Niveau de preuve : code pays fourni par la source.

Le résumé fourni par la source

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.

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Le contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.

Titre Crossref
The Solar Orbiter Science Activity Plan
Date Crossref
30/09/2020
Éditeur
EDP Sciences
Type
journal-article

Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.

Les institutions déclarées

European Space Astronomy CentreEuropean Space Research and Technology CentreGoddard Space Flight CenterHeliophysicsCentre National de la Recherche ScientifiqueUniversité Paris-SaclayInstitut d'Astrophysique SpatialeRoyal Observatory of BelgiumRutherford Appleton LaboratoryImperial College LondonUnited States Naval Research LaboratoryNaval Research Laboratory Space Science DivisionFHNW University of Applied Sciences and Arts Northwestern SwitzerlandUniversité Paris CitéUniversité Paris Sciences et LettresObservatoire de ParisSorbonne UniversitéLaboratoire d’études spatiales et d’instrumentation en astrophysiqueUniversity College LondonUniversidad de AlcaláUniversity of FlorenceKyung Hee UniversityMax Planck Institute for Solar System ResearchOsservatorio Astrofisico di TorinoNational Observatory of AthensAstronomical Observatory of CapodimonteUniversitat de BarcelonaUniversity of California, BerkeleyInstituto de Astrofísica de AndalucíaÉcole PolytechniqueLaboratoire de Physique des PlasmasCommissariat à l'Énergie Atomique et aux Énergies AlternativesAstrophysique, Instrumentation et ModélisationSorbonne Paris CitéCEA Paris-SaclayInstitute for Space Astrophysics and PlanetologyTechnische Universität BerlinSouthwest Research InstituteQueen Mary University of LondonUniversité Toulouse III - Paul SabatierUniversité Fédérale de Toulouse Midi-PyrénéesInstitut de Recherche en Astrophysique et PlanétologieOsservatorio Astrofisico di CataniaUniversité d'OrléansLaboratoire de Physique et Chimie de l’Environnement et de l’EspaceGeorgia State UniversityAcademy of AthensPhysikalisch-Meteorologisches Observatorium DavosETH ZurichJohns Hopkins University Applied Physics LaboratoryNorthumbria UniversityKU LeuvenSwedish Institute of Space PhysicsUniversity of GlasgowLeibniz Institute for Astrophysics PotsdamUniversity of MichiganJet Propulsion LaboratoryPredictive Science (United States)Dublin Institute For Advanced StudiesTrinity College DublinNational Solar ObservatoryUniversité Bourgogne Franche-ComtéUniversity of ArizonaUniversity of IoanninaUniversity of ReadingArcetri Astrophysical ObservatoryAgenzia Spaziale ItalianaTechnische Universität DresdenUniversity of LiègeInstitut für SonnenphysikInstitute for the Science and Technology of PlasmasNational Polytechnic SchoolCzech Academy of Sciences, Institute of Atmospheric PhysicsAustrian Academy of SciencesSpace Research InstituteCzech Academy of Sciences, Astronomical InstituteChristian-Albrechts-Universität zu KielUniversidad de MurciaUniversity of CalabriaKTH Royal Institute of TechnologyRadboud University NijmegenUniversity of New HampshireLomonosov Moscow State University

Une affiliation ne permet pas de déduire la nationalité d’un auteur.

Les sujets associés

Solar and Space Plasma DynamicsAstro and Planetary SciencePlanetary Science and Exploration

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