Hue, V.; Greathouse, T. K.; Cavalié, T.; Dobrijevic, M.; Hersant, F.: 2D photochemical modeling of Saturn's stratosphere. Part II: Feedback between composition and temperature. Icarus 267, pp. 334 - 343 (2016)
Cavalié, T.; Dobrijevic, M.; Fletcher, L. N.; Loison, L.-C.; Hickson, K. M.; Hue, V.; Hartogh, P.: Photochemical response to the variation of temperature in the 2011-2012 stratospheric vortex of Saturn. Astronomy and Astrophysics 580, A55 (2015)
Hue, V.; Cavalié, T.; Dobrijevic, M.; Hersant, F.; Greathouse, T. K.: 2D photochemical modeling of Saturn's stratosphere. Part I: Seasonal variation of atmospheric composition without meridional transport. Icarus 257, pp. 163 - 184 (2015)
Lellouch, E.; Moreno, R.; Orton, G. S.; Feuchtgruber, H.; Cavalié, T.; Moses, J. I.; Hartogh, P.; Jarchow, C.; Sagawa, H.: New constraints on the CH4 vertical profile in Uranus and Neptune from Herschel observations. Astronomy and Astrophysics 579, A121 (2015)
Mandt, K. E.; Mousis, O.; Marty, B.; Cavalié, T.; Harris, W.; Hartogh, P.; Willacy, K.: Constraints from Comets on the Formation and Volatile Acquisition of the Planets and Satellites. Space Science Reviews 197, pp. 297 - 342 (2015)
Hickson, K. M.; Loison, J. C.; Cavalié, T.; Hébrard, É.; Dobrijevic, M.: The evolution of infalling sulfur species in Titan's atmosphere. Astronomy and Astrophysics 572, A58 (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)
Cavalié, T.; Hartogh, P.; Billebaud, F.; Dobrijevic, M.; Fouchet, T.; Lellouch, E.; Encrenaz, T.; Brillet, J.; Moriarty-Schieven, G. H.: A cometary origin for CO in the stratosphere of Saturn? Astronomy and Astrophysics 510, A88 (2010)
Dobrijevic, M.; Cavalié, T.; Hebrard, E.; Billebaud, F.; Hersant, F.; Selsis, F.: Key reactions in the photochemistry of hydrocarbons in Neptune's stratosphere. Planetary and Space Science 58 (12), pp. 1555 - 1566 (2010)
Hartogh, P.; Crovisier, J.; de Val-Borro, M.; Bockelée-Morvan, D.; Biver, N.; Lis, D. C.; Moreno, R.; Jarchow, C.; Rengel, M.; Emprechtinger, M.et al.; Szutowicz, S.; Banaszkiewicz, M.; Blecka, M. I.; Cavalié, T.; Encrenaz, T.; Jehin, E.; Küppers, M.; Lara, L.-M.; Lellouch, E.; Swinyard, B. M.; Vandenbussche, B.; Bergin, E. A.; Blake, G. A.; Blommaert, J. A. D. L.; Cernicharo, J.; Decin, L.; Encrenaz, P.; de Graauw, T.; Hutsemekers, M.; Kidger, M.; Manfroid, J.; Medvedev, A.; Naylor, D. A.; Schieder, R.; Thomas, N.; Waelkens, C.; Roelfsema, P. R.; Dieleman, P.; Güsten, R.; Klein, T.; Kasemann, C.; Caris, M.; Olberg, M.; Benz, A. O.: HIFI observations of water in the atmosphere of comet C/2008 Q3 (Garradd). Astronomy and Astrophysics 518, L150 (2010)
Hartogh, P.; Jarchow, C.; Lellouch, E.; de Val-Borro, M.; Rengel, M.; Moreno, R.; Medvedev, A. S.; Sagawa, H.; Swinyard, B. M.; Cavalié, T.et al.; Lis, D. C.; Błecka, M. I.; Banaszkiewicz, M.; Bockelée-Morvan, D.; Crovisier, J.; Encrenaz, T.; Küppers, M.; Lara, L.-M.; Szutowicz, S.; Vandenbussche, B.; Bensch, F.; Bergin, E. A.; Billebaud, F.; Biver, N.; Blake, G. A.; Blommaert, J. A. D. L.; Cernicharo, J.; Decin, L.; Encrenaz, P.; Feuchtgruber, H.; Fulton, T.; de Graauw, T.; Jehin, E.; Kidger, M.; Lorente, R.; Naylor, D. A.; Portyankina, G.; Sánchez-Portal, M.; Schieder, R.; Sidher, S.; Thomas, N.; Verdugo, E.; Waelkens, C.; Whyborn, N.; Teyssier, D.; Helmich, F.; Roelfsema, P.; Stutzki, J.; Leduc, H. G.; Stern, J. A.: Herschel/HIFI observations of Mars: First detection of O2 at submillimetre wavelengths and upper limits on HCl and H2O2. Astronomy and Astrophysics 521, L49 (2010)
Sagawa, H.; Hartogh, P.; Rengel, M.; de Lange, A.; Cavalié, T.: Preparation for the solar system observations with Herschel: Simulation of Jupiter observations with PACS. Planetary and Space Science 58, pp. 1692 - 1698 (2010)
Sagawa, H.; Hartogh, P.; Rengel, M.; Lange, A.; Cavalié, T.: Preparation for the solar system observations with Herschel: Simulation of Jupiter observations with PACS. Planetary and Space Science 58 (13), pp. 1692 - 1698 (2010)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
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 magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.