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The Radio & Plasmas Waves instrument on the Solar Orbiter mission : science objectives and capabilities

Authors :
Maksimovic, M.
Krasnoselskikh, V.
Bale, S. D.
Soucek, J.
Vaivads, A.
Chust, Thomas
Steller, M.
Travnicek, Pavel
Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire de Physique des Plasmas (LPP)
Université Paris-Saclay-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-École polytechnique (X)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)
Swedish Institute of Space Physics [Uppsala] (IRF)
Université Paris-Sud - Paris 11 (UP11)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École polytechnique (X)-Sorbonne Université (SU)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)
Source :
American Astronomical Society, SPD meeting #48, American Astronomical Society, SPD meeting #48, Aug 2017, Portland, Oregon, United States. pp.110.05, 40th COSPAR Scientific Assembly, 40th COSPAR Scientific Assembly, Aug 2014, Moscou, Russia. pp.D2.3-29-14
Publication Year :
2017
Publisher :
HAL CCSD, 2017.

Abstract

International audience; We will review the science objectives of the Radio & Plasmas Waves (RPW) instrument on the Solar Orbiter mission. Among those the study of the connectivity between the solar corona and the inner Heliosphere as close as from 0.3 AU and the kinetic behavior of the Solar Wind are of prime importance. We present then the RPW technical capabilities which will allow in-situ and remote sensing measurements of both electrostatic and electromagnetic fields and waves in a broad frequency range, typically from a fraction of Hertz to a few tens of MHz.

Details

Language :
English
Database :
OpenAIRE
Journal :
American Astronomical Society, SPD meeting #48, American Astronomical Society, SPD meeting #48, Aug 2017, Portland, Oregon, United States. pp.110.05, 40th COSPAR Scientific Assembly, 40th COSPAR Scientific Assembly, Aug 2014, Moscou, Russia. pp.D2.3-29-14
Accession number :
edsair.dedup.wf.001..42de905d43c346f71dd5252c9679bc36