EGU25-16581, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-16581
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Tuesday, 29 Apr, 08:35–08:45 (CEST)
 
Room L1
Visiting the emptiest space – Analysing the JUICE Lunar flyby PEP-JDC data 
Philipp Wittmann1, Martin Wieser1, Stas Barabash1, Gabriella Stenberg Wieser1, Thomas Maynadié1, Norbert Krupp2, Elias Roussos2, Markus Fränz2, Pontus Brandt3, Peter Wurz4, Jasper Halekas5, Andrew Poppe6, and the PEP Team*
Philipp Wittmann et al.
  • 1Swedish Institute of Space Physics, Kiruna, Sweden (philipp.wittmann@irf.se)
  • 2Max Planck Institute for Solar System Research, Göttingen, Germany
  • 3Applied Physics Laboratory, Johns Hopkins University, Laurel, USA
  • 4University Bern, Physikalisches Institut, Bern, Switzerland
  • 5University of Iowa, Iowa City, USA
  • 6University of California, Berkeley, USA
  • *A full list of authors appears at the end of the abstract

The JUpiter ICy moons Explorer (JUICE) performed end of August 2024 its Lunar-Earth gravity assist consisting of a flyby of the Moon followed by an Earth flyby. During this manoeuvre the Particle Environment Package (PEP) was operated to investigate both the near lunar and the magnetospheric environment and to validate its performance. PEP consists of six individual sensors detecting ions, electrons and ENAs depending on their energy, arrival direction and mass. Here we focus on measurements of one of these sensors, the Jovian plasma Dynamics and Composition analyzer (JDC). JDC measures angular and mass-resolved positive and negative ions as well as electrons in an energy range from a few eV/q up to 35 keV/q. The JDC field of view covers a hemisphere and is divided into 16 x 12 angular pixels.

We present JDC data from the lunar flyby. During the flyby, the Moon was in Earth’s magnetotail. JUICE approached the moon from the side of the lunar wake. JDC was operated for ~103 minutes during the flyby with the exception of an 8 minutes long period around the closest approach to the Moon. The observed plasma densities during the lunar flyby were extremely low - making this region one of the emptiest spaces. Nevertheless, after entering the lunar optical shadow until the end of the measurement interval a weak signal at ~1.5 keV/q was detected. This signal is not an instrument background and is not visible before entering the Lunar optical shadow. We show ray tracing results to investigate the possible origin of these particles.

PEP Team:

All PEP team members

How to cite: Wittmann, P., Wieser, M., Barabash, S., Stenberg Wieser, G., Maynadié, T., Krupp, N., Roussos, E., Fränz, M., Brandt, P., Wurz, P., Halekas, J., and Poppe, A. and the PEP Team: Visiting the emptiest space – Analysing the JUICE Lunar flyby PEP-JDC data , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16581, https://doi.org/10.5194/egusphere-egu25-16581, 2025.