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An overview of the results obtained so far with the Radio Plasma Waves instrument onboard Solar Orbiter

Authors

Kretzschmar,  Matthieu
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Maksimovic,  Milan
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Colomban,  Lucas
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Krasnoselskikh,  Volodya
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Chust,  Thomas
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Khotyaintsev,  Yuri
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Soucek,  Jan
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Vecchio,  Antonio
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

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Citation

Kretzschmar, M., Maksimovic, M., Colomban, L., Krasnoselskikh, V., Chust, T., Khotyaintsev, Y., Soucek, J., Vecchio, A. (2023): An overview of the results obtained so far with the Radio Plasma Waves instrument onboard Solar Orbiter, XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG) (Berlin 2023).
https://doi.org/10.57757/IUGG23-4373


Cite as: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5021804
Abstract
The Radio Plasma Waves instrument onboard Solar Orbiter measures the electomagnetic fields from a 1 Hz (and DC for the electric field) to a few MHz. Since the launch of Solar Orbiter in 2018, RPW has monitored solar radio burst, in situ waves (whistler, ion-accoustic, Langmuir, ..), dust and turbulence. We will present an overview of the obtained results, with an emphasis on the ones obtained using the search coil magnetometer : whistler waves and their impact on solar wind electrons populations, turbulence, and high frequency electromagnetic waves.