Kotova, A.; Roussos, E.; Krupp, N.; Dandouras, I.: Galactic Cosmic Rays access to the upper atmosphere and rings of Saturn. AGU Fall Meeting, San Francisco, USA (2016)
Regoli, L. H.; Roussos, E.; Luhmann, J.; Dialynas, K.; Krupp, N.; Jones, G. H.; Coates, A. J.: Energetic environment at Titan's orbit. AGU Fall Meeting, San Francisco, USA (2016)
Lee-Payne, Z.; Grande, M.; Krupp, N.; Paranicas, C.; Roussos, E.; Kollmann, P.: Re-evaluating Galileo Energetic Particle Detector data based on radiation detector decay; for use in estimating Sputtering Erosion rates on Europa. European Planetary Science Congress EPSC , Nantes, France (2015)
Palmaerts, B.; Roussos, E.; Krupp, N.; Kurth, W. S.; Mitchell, D. G.; Dougherty, M. K.: Statistical analysis and multi-instrument overview of the quasi-periodic 1-hour pulsations in Saturn's outer magnetosphere. European Planetary Science Congress EPSC , Nantes, France (2015)
Regoli, L.; Coates, A.; Thomsen, M.; Feyerabend, M.; Jones, G.; Roussos, E.; Krupp, N.: Pickup Ion Signatures in the Vicinity of Titan. AGU Fall Meeting, San Francisco, USA (2015)
Roussos, E.; Krupp, N.; Fraenz, M.; Kollmann, P.; Truscott, P.; Futaana, Y.: Hot Plasma Environment Model (HPEM): A empirical model for describing time-dependent processes of the jovian energetic electron environment. European Planetary Science Congress EPSC , Nantes, France (2015)
Regoli, L.; Feyerabend, M.; Kotova, A.; Roussos, E.; Jones, G.; Krupp, N.; Coates, A.: Mapping the flow of energetic particles in Titan's exobase. European Planetary Science Congress EPSC, Cascais, Portugal (2014)
Regoli, L.; Feyerabend, M.; Kotova, A.; Roussos, E.; Jones, G.; Krupp, N.; Coates, A.: Tracing of energetic particles in the vicinity of Titan. European Geosciences Union General Assembly, Vienna, Austria (2014)
Regoli, L.; Feyerabend, M.; Kotova, A.; Roussos, E.; Jones, G.; Krupp, N.; Coates, A.: Mapping the flow of energetic particles in Titan's exobase. 10 years of Cassini-Huygens in the Saturnian system, London, UK (2014)
Krupp, N.: Drei-dimensionale Richtungsverteilungen und relative Häufigkeiten energiereicher Ionen in der Magnetosphäre des Jupiter. Dissertation, Technische Universität Braunschweig (1994)
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
The MPS instruments on board ESA’s JUICE spacecraft have successfully completed their commissioning in space - and delivered their first observational data.
A collision nearly 30 years ago permanently changed Jupiter's atmospheric chemistry; the aftermath is still helping to better understand the gas giant.
The launch was successful; the ESA’s space probe JUICE is now on its way to the Jupiter system. There, it will primarily study the gas giant's icy moons.
ESA's space probe is on the move: First it heads for the launch site in Kourou - and in April it will begin its long journey to Jupiter and its icy moons.