Maksimovic, M;
Bale, SD;
Chust, T;
Khotyaintsev, Y;
Krasnoselskikh, V;
Kretzschmar, M;
Plettemeier, D;
... Vaivads, A; + view all
(2020)
The Solar Orbiter Radio and Plasma Waves (RPW) instrument.
Astronomy & Astrophysics
10.1051/0004-6361/201936214.
(In press).
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Abstract
The Radio and Plasma Waves (RPW) instrument on the ESA Solar Orbiter mission is described in this paper. This instrument is designed to measure in-situ magnetic and electric fields and waves from the continuous to a few hundreds of kHz. RPW will also observe solar radio emissions up to 16 MHz. The RPW instrument is of primary importance to the Solar Orbiter mission and science requirements since it is essential to answer three of the four mission overarching science objectives. In addition RPW will exchange on-board data with the other in-situ instruments in order to process algorithms for interplanetary shocks and type III langmuir waves detections.
Type: | Article |
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Title: | The Solar Orbiter Radio and Plasma Waves (RPW) instrument |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1051/0004-6361/201936214 |
Publisher version: | https://doi.org/10.1051/0004-6361/201936214 |
Language: | English |
Additional information: | This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions. |
Keywords: | Solar Wind, space instrumentation, plasma and radio waves |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics |
URI: | https://discovery-pp.ucl.ac.uk/id/eprint/10110663 |
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