EGU21-8959
https://doi.org/10.5194/egusphere-egu21-8959
EGU General Assembly 2021
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

Dust Grain Detection by Solar Orbiter, Parker Solar Probe, and Magnetospheric Multiscale (MMS) Mission — Similarities and Differences

Jakub Vaverka1, Jiří Pavlů1, Libor Nouzák1, Samuel Kočiščák1, Jana Šafránková1, Zdeněk Němeček1, David Píša2, Jan Souček2, Arnaud Zaslavsky3, Ingrid Mann4, Milan Maksimovic5, Stuart Bale6, and Per-Arne Linqvist7
Jakub Vaverka et al.
  • 1Faculty of Mathematics and Physics, Charles University, Prague, Czechia (jakub.vaverka@mff.cuni.cz)
  • 2Institute of Atmospheric Physics of the Czech Academy of Sciences, Prague, Czech Republic
  • 3LESIA – Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, France
  • 4Institute of Physics and Technology, UiT, Arctic University of Norway, Tromso, Norway
  • 5LESIA, Observatoire de Paris, France
  • 6University of California, Berkeley, USA
  • 7Royal Institute of Technology, Stockholm, Sweden

The dust impact detection by electric field instruments is already a well-established technique. On the other hand, not all aspects of signal generation by dust impacts and its consequent detection are completely understood and explained. It has been shown that the design and configuration (monopole/dipole) of the electric field antennas/probes are very important for dust impact detection and understanding of the measured signal. Therefore, it is not straightforward to compare detected signals by various spacecraft. Most of space missions use at the same time either monopole or dipole antenna configuration. However, the MMS simultaneous monopole and dipole measurements provide us with interesting information about dust impact signals. We have analyzed individual electric field waveforms of dust impacts detected by Solar Orbiter, Parker Solar Probe, and MMS to understand similarities and differences of dust detection by various spacecraft with different antenna designs and configurations. This understanding will allow us to reliably compare obtained dust fluxes among individual missions.  

How to cite: Vaverka, J., Pavlů, J., Nouzák, L., Kočiščák, S., Šafránková, J., Němeček, Z., Píša, D., Souček, J., Zaslavsky, A., Mann, I., Maksimovic, M., Bale, S., and Linqvist, P.-A.: Dust Grain Detection by Solar Orbiter, Parker Solar Probe, and Magnetospheric Multiscale (MMS) Mission — Similarities and Differences, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-8959, https://doi.org/10.5194/egusphere-egu21-8959, 2021.

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