Research Group "Planetary Plasma Environment" (Sept 2015)

<p style="margin: 0cm 0cm 1em;"><span style="color: #444444; font-family: 'Verdana','sans-serif'; font-size: 9.5pt; mso-ansi-language: DE;" lang="DE">left to right: Leonardo Regoli (now at UMICH), Dr. Kun Li (now at Beijing University), Sibylla Siebert-Rust, Dr. Patrick Daly, Anna Kotova (now at IRAP, Toulouse), Benjamin Palmaerts, Dr. Elias Roussos, Dr. Markus Fränz, Dr. Norbert Krupp, <span style="color: #444444; font-family: 'Verdana','sans-serif'; font-size: 9.5pt;">Prof. Eduard Dubinin, </span>Dr. Elena Kronberg, Dr. Esa Villenius.<br /> </span></p>
<p style="margin: 0cm 0cm 1em;"><span style="color: #444444; font-family: 'Verdana','sans-serif'; font-size: 9.5pt;">Missing in picture: Dr. Harald Krüger, Dr. Stein Haaland, Mikhail Rashev</span></p> Zoom Image

left to right: Leonardo Regoli (now at UMICH), Dr. Kun Li (now at Beijing University), Sibylla Siebert-Rust, Dr. Patrick Daly, Anna Kotova (now at IRAP, Toulouse), Benjamin Palmaerts, Dr. Elias Roussos, Dr. Markus Fränz, Dr. Norbert Krupp, Prof. Eduard Dubinin, Dr. Elena Kronberg, Dr. Esa Villenius.

Missing in picture: Dr. Harald Krüger, Dr. Stein Haaland, Mikhail Rashev

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Contact

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Sibylla Siebert-Rust
Secretary
Phone:+49 551 384 979-424

daily 8:00-12:30 h

Research Group "Planetary Plasma Environment"

Research Group "Planetary Plasma Environment" PPE

Welcome to the "Planetary Plasma Environment" Research Group (PPE) at the Max Planck Institute for Solar System Research

The PPE-Research Group is studying neutral and charged particles in the vicinity of the planets and their moons.

We study the interaction of surfaces/atmospheres/exospheres of planets or moons with the surrounding plasma (solar wind or magnetosphere) in detail.

The PPE group uses data from instruments onboard spacecraft, some of them designed and developed at MPS as well as Hybrid simulations.

Currently the following research topics are studied in detail:

  • Investigation of neutral and charged particle populations in the vicinity of Mercury, Venus, Earth, Mars, Jupiter, and Saturn based on available data sets.

  • Plasma und neutral gas in the magnetospheres of Jupiter and Saturn including "neutral particle imaging"
  • Investigation of the radiation belts of the Earth, Jupiter, Saturn
  • Interaction between plasma and atmosphere/surfaces of planets and their moons (currently focused on Saturn)
  • Hybrid simulations of the Plasma-Planet/Moon interaction
  • Dust distribution in the vicinity of the Galilean moons
  • Interstellar dust in the solar system
 
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