1. The Energetic Particle Detector. Energetic particle instrument suite for the Solar Orbiter mission
- Author
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Milan Maksimovic, G. M. Mason, M. E. Wiedenbeck, S. Kolbe, Pertti Makela, A. Ravanbakhsh, N. Vilmer, C. Gordillo, L. Seimetz, Lauri Panitzsch, A. da Silva Fariña, A. Russu, R. Elftmann, Stephan Böttcher, J. R. Hayes, R. Paspirgilis, Aarón Montalvo, S. Begley, Säm Krucker, Óscar Ramón Ramos Gutiérrez, Pablo Parra, Alberto Carrasco, Eduard P. Kontar, Andrew Walsh, Sebastián Sánchez-Prieto, Stefan J. Hofmeister, Karl-Ludwig Klein, J. Tammen, E. Böhm, Olga Malandraki, B. Schuster, K. S. Nelson, F. Espinosa Lara, Jia Yu, Manuel Prieto, Arik Posner, W. Dröge, Neus Agueda, O. Gevin, I. Sánchez, Raúl Gómez-Herrero, C. Terasa, K. Tyagi, Rami Vainio, A. R. Dupont, Juan Jose Blanco, C. E. Schlemm, Angels Aran, Q. Zong, James M. Ryan, A. Kulemzin, Matthew E. Hill, David Lario, Jan Soucek, Jan Köhler, Cesar Martin, Karel Kudela, Robert F. Wimmer-Schweingruber, G. C. Ho, S. Kerem, Javier Rodriguez-Pacheco, T. I. Varela, O. Rodríguez-Polo, D. Meziat, Bernd Heber, O. Limousin, K. Wirth, V. Knierim, D. Pacheco, V. de Manuel González, H. Seifert, J. Almena, Christopher J. Owen, Yulia Kartavykh, Shrinivasrao R. Kulkarni, S. Boden, A. Martínez Hellín, J. J. Connell, S. Eldrum, Christian Drews, H. Önel, I. Cernuda, R. Castillo, Natchimuthuk Gopalswamy, S. Liang, W. J. Lees, Dennis Haggerty, M. Jüngling, Linghua Wang, W. Boogaerts, Silvia Dalla, B. Klecker, Timothy S. Horbury, M. Yedla, M. L Richards, G. B. Andrews, Jan Steinhagen, Blai Sanahuja, G. Mann, Universidad de Alcalá - University of Alcalá (UAH), Institut für Experimentelle und Angewandte Physik [Kiel] (IEAP), Christian-Albrechts-Universität zu Kiel (CAU), Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL), Universidad de Tarapaca, Paul Scherrer Institute (PSI), Indian Institute of Technology Bombay (IIT Bombay), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), and Science and Technology Facilities Council (STFC)
- Subjects
Sun: flares ,010504 meteorology & atmospheric sciences ,Sun: coronal mass ejections (CMEs) ,Population ,Astrophysics ,Astronomy & Astrophysics ,FOCUSED TRANSPORT ,01 natural sciences ,Particle detector ,Particle identification ,law.invention ,Orbiter ,law ,Sun: particle emission ,0201 Astronomical and Space Sciences ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Sun: heliosphere ,education ,010303 astronomy & astrophysics ,acceleration of particles ,HIGH-ENERGIES ,0105 earth and related environmental sciences ,Physics ,education.field_of_study ,Science & Technology ,INTERPLANETARY SHOCKS ,Solar energetic particles ,instrumentation: detectors ,Ecliptic ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,Astronomy and Astrophysics ,COSMIC-RAYS ,ADIABATIC DECELERATION ,CORONAL MASS EJECTIONS ,SPACECRAFT OBSERVATIONS ,Space and Planetary Science ,[SDU]Sciences of the Universe [physics] ,Physical Sciences ,Physics::Space Physics ,SEP EVENTS ,Heliospheric current sheet ,Astrophysics::Earth and Planetary Astrophysics ,PROTON PEAK INTENSITIES ,MONTE-CARLO SIMULATIONS ,Heliosphere - Abstract
International audience; After decades of observations of solar energetic particles from space-based observatories, relevant questions on particle injection, transport, and acceleration remain open. To address these scientific topics, accurate measurements of the particle properties in the inner heliosphere are needed. In this paper we describe the Energetic Particle Detector (EPD), an instrument suite that is part of the scientific payload aboard the Solar Orbiter mission. Solar Orbiter will approach the Sun as close as 0.28 au and will provide extra-ecliptic measurements beyond ∼30° heliographic latitude during the later stages of the mission. The EPD will measure electrons, protons, and heavy ions with high temporal resolution over a wide energy range, from suprathermal energies up to several hundreds of megaelectronvolts/nucleons. For this purpose, EPD is composed of four units: the SupraThermal Electrons and Protons (STEP), the Electron Proton Telescope (EPT), the Suprathermal Ion Spectrograph (SIS), and the High-Energy Telescope (HET) plus the Instrument Control Unit that serves as power and data interface with the spacecraft. The low-energy population of electrons and ions will be covered by STEP and EPT, while the high-energy range will be measured by HET. Elemental and isotopic ion composition measurements will be performed by SIS and HET, allowing full particle identification from a few kiloelectronvolts up to several hundreds of megaelectronvolts/nucleons. Angular information will be provided by the separate look directions from different sensor heads, on the ecliptic plane along the Parker spiral magnetic field both forward and backwards, and out of the ecliptic plane observing both northern and southern hemispheres. The unparalleled observations of EPD will provide key insights into long-open and crucial questions about the processes that govern energetic particles in the inner heliosphere.
- Published
- 2020
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