Issue |
A&A
Volume 642, October 2020
The Solar Orbiter mission
|
|
---|---|---|
Article Number | A7 | |
Number of page(s) | 35 | |
Section | Astronomical instrumentation | |
DOI | https://doi.org/10.1051/0004-6361/201935287 | |
Published online | 30 September 2020 |
The Energetic Particle Detector
Energetic particle instrument suite for the Solar Orbiter mission
1
Universidad de Alcalá, Space Research Group, 28805 Alcalá de Henares, Spain
e-mail: javier.pacheco@uah.es
2
Institut für Experimentelle und Angewandte Physik, Christian-Albrechts-Universität zu Kiel, Kiel, Germany
3
Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA
4
University of Colorado/LASP, Boulder, CO, USA
5
Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona, Barcelona, Spain
6
Imperial College London, UK
7
ESA-ESAC, Madrid, Spain
8
Observatoire de Paris-Meudon, France
9
Karl-Franzens-Universität Graz, Austria
10
Institute of Atmospheric Physics, Prague, Czech Republic
11
University of New Hampshire, Durham, USA
12
NASA HQ, Washington DC, USA
13
University of Peking, PR China
14
ESA-ESTEC, Noordwijk, The Netherlands
15
Jet Propulsion Laboratory, Pasadena, CA, USA
16
Max-Planck-Institut für extraterrestrische Physik, Garching, Germany
17
School of Physics & Astronomy, University of Glasgow, UK
18
Windisch, Switzerland & SSL, UC, Berkeley, USA
19
National Observatory of Athens/IAASARS, Greece
20
University College, London, UK
21
University of Turku, Turku, Finland
22
University of Central Lancashire, UK
23
University of Würzburg, Germany
24
Commissariat à l’énergie atomique, CEA Saclay, France
25
Institute of Experimental Physics, Slovak Academy of Sciences, Slovakia
26
Goddard Space Flight Center, Greenbelt, MD, USA
27
Leibniz-Institut für Astrophysik Potsdam (AIP), Potsdam, Germany
28
Ioffe Physical-Technical Institute, St-Petersburg, Russia
Received:
15
February
2019
Accepted:
15
April
2019
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.
Key words: acceleration of particles / instrumentation: detectors / Sun: coronal mass ejections (CMEs) / Sun: flares / Sun: heliosphere / Sun: particle emission
© ESO 2020
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