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de Val-Borro, M.; Bockelée-Morvan, D.; Jehin, E.; Hartogh, P.; Opitom, C.; Szutowicz, S.; Biver, N.; Crovisier, J.; Lis, D. C.; Rezac, L.et al.; de Graauw, T.; Hutsemékers, D.; Jarchow, C.; Kidger, M.; Küppers, M.; Lara, L. M.; Manfroid, J.; Rengel, M.; Swinyard, B. M.; Teyssier, D.; Vandenbussche, B.; Waelkens, C.: Herschel observations of gas and dust in comet C/2006 W3 (Christensen) at 5 AU from the Sun. Astronomy and Astrophysics 564, A124 (2014)
Lara, L. M.; Lellouch, E.; González, M.; Moreno, R.; Rengel, M.: A time‐dependent photochemical model for Titan's atmosphere and the origin of H2O. Astronomy and Astrophysics 566, A143 (2014)
Rezac, L.; de Val-Borro, M.; Hartogh, P.; Cavalié, T.; Jarchow, C.; Rengel, M.; Dobrijevic, M.: New determination of the HCN profile in the stratosphere of Neptune from millimeter-wave spectroscopy. Astronomy and Astrophysics 563, A4 (2014)
Lis, D. C.; Biver, N.; Bockelée-Morvan, D.; Hartogh, P.; Bergin, E. A.; Blake, G. A.; Crovisier, J.; de Val-Borro, M.; Jehin, E.; Küppers, M.et al.; Manfroid, J.; Moreno, R.; Rengel, M.; Szutowicz, S.: A Herschel Study of D/H in Water in the Jupiter-family comet 45P/Honda-Mrkos-Pajdušáková and Prospects for D/H Measurements with CCAT. Astrophysical Journal 774, L3 (2013)
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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).