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First observations and performance of the RPW instrument on board the Solar Orbiter mission

  • M. Maksimovic
  • , J. Souček
  • , T. Chust
  • , Y. Khotyaintsev
  • , M. Kretzschmar
  • , X. Bonnin
  • , A. Vecchio
  • , O. Alexandrova
  • , S. D. Bale
  • , D. Bérard
  • , J. Y. Brochot
  • , N. J.T. Edberg
  • , A. Eriksson
  • , L. Z. Hadid
  • , E. P.G. Johansson
  • , T. Karlsson
  • , B. Katra
  • , V. Krasnoselskikh
  • , V. Krupař
  • , S. Lion
  • E. Lorfèvre, L. Matteini, Q. N. Nguyen, D. Píša, R. Piberne, D. Plettemeier, H. O. Rucker, O. Santolík, K. Steinvall, M. Steller, Štverák, P. Trávníček, A. Vaivads, A. Zaslavsky, S. Chaintreuil, M. Dekkali, P. A. Astier, G. Barbary, K. Boughedada, B. Cecconi, F. Chapron, C. Collin, D. Dias, L. Guéguen, L. Lamy, V. Leray, L. R. Malac-Allain, F. Pantellini, J. Parisot, P. Plasson, S. Thijs, I. Fratter, E. Bellouard, P. Danto, S. Julien, E. Guilhem, C. Fiachetti, J. Sanisidro, C. Laffaye, F. Gonzalez, B. Pontet, N. Quéruel, G. Jannet, P. Fergeau, T. Dudok De Wit, T. Vincent, C. Agrapart, J. Pragout, M. Bergerard-Timofeeva, G. T. Delory, P. Turin, A. Jeandet, P. Leroy, J. C. Pellion, V. Bouzid, W. Recart, I. Kolmašová, O. Krupařová, L. Uhlíř, R. Lán, J. Baše, M. André, L. Bylander, V. Cripps, C. Cully, S. E. Jansson, W. Puccio, J. Břínek, H. Ottacher, V. Angelini, M. Berthomier, V. Evans, K. Goetz, P. Hellinger, T. S. Horbury, K. Issautier, E. Kontar, O. Le Contel, P. Louarn, M. Martinović, D. Müller, H. O'brien, C. J. Owen, A. Retino, J. Rodríguez-Pacheco, F. Sahraoui, L. Sanchez, A. P. Walsh, R. F. Wimmer-Schweingruber, I. Zouganelis
  • Sorbonne Univ.
  • Institute of Atmospheric Physics of the Academy of Sciences of the Czech Republic
  • Sorbonne Université
  • Swedish Institute of Space Physics
  • CNRS
  • conventionnée avec l'Université d'Orléans
  • Radboud University
  • University of California, Space Sciences Laboratory
  • University of California, Berkeley
  • Stellar Scientific (Now HELIOSPACE)
  • KTH Royal Institute of Technology
  • Biochemical and Environmental Engineering
  • NASA Goddard Space Flight Center
  • Centre National d'études Spatiales
  • Imperial College London
  • Technical University Dresden
  • IMBA Institute of Molecular Biotechnology of the Austrian Academy of Sciences
  • Charles University
  • Space Research Institute
  • Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i.
  • LAM
  • Nexeya Conseil & Formation
  • Capgemini Engineering
  • University of Rennes
  • University of Calgary
  • University of Minnesota
  • University of Glasgow
  • IRAP/CNRS
  • University of Arizona
  • University of Belgrade
  • ESTEC - European Space Research and Technology Centre
  • UCL Mullard Space Science Laboratory
  • Universidad de Alcalá
  • ESAC campus
  • Christian-Albrechts-University Kiel

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

The Radio and Plasma Waves (RPW) instrument on the ESA Solar Orbiter mission is designed to measure in situ magnetic and electric fields and waves from the continuum up to several hundred kHz. The RPW also observes solar and heliospheric radio emissions up to 16 MHz. It was switched on and its antennae were successfully deployed two days after the launch of Solar Orbiter on February 10, 2020. Since then, the instrument has acquired enough data to make it possible to assess its performance and the electromagnetic disturbances it experiences. In this article, we assess its scientific performance and present the first RPW observations. In particular, we focus on a statistical analysis of the first observations of interplanetary dust by the instrument's Thermal Noise Receiver. We also review the electro-magnetic disturbances that RPW suffers, especially those which potential users of the instrument data should be aware of before starting their research work.

langue originaleAnglais
Numéro d'articleA41
journalAstronomy and Astrophysics
Volume656
Les DOIs
étatPublié - 1 déc. 2021

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