Ball, W. H.; Gizon, L.: A new correction of stellar oscillation frequencies for near-surface effects (Corrigendum). Astronomy and Astrophysics 569, C2 (2014)
Cameron, R. H.; Jiang, J.; Schuessler, M.; Gizon, L.: Physical causes of solar cycle amplitude variability. Journal of Geophysical Research: Space Physics 119, pp. 680 - 688 (2014)
Deheuvels, S.; Doğan, G.; Goupil, M. J.; Appourchaux, T.; Benomar, O.; Bruntt, H.; Campante, T. L.; Casagrande, L.; Ceillier, T.; Davies, G. R.et al.; De Cat, P.; Fu, J. N.; García, R. A.; Lobel, A.; Mosser, B.; Reese, D. R.; Regulo, C.; Schou, J.; Stahn, T.; Thygesen, A. O.; Yang, X. H.; Chaplin, W. J.; Christensen-Dalsgaard, J.; Eggenberger, P.; Gizon, L.; Mathis, S.; Molenda-Żakowicz, J.; Pinsonneault, M.: Seismic constraints on the radial dependence of the internal rotation profiles of six Kepler subgiants and young red giants. Astronomy and Astrophysics 564, A27 (2014)
Fournier, D.; Gizon, L.; Hohage, T.; Birch, A.: Generalization of the noise model for time‐distance helioseismology. Astronomy and Astrophysics 567, A137 (2014)
Jiang, J.; Hathaway, D. H.; Cameron, R. H.; Solanki, S. K.; Gizon, L.; Upton, L.: Magnetic Flux Transport at the Solar Surface. Space Science Reviews 186, pp. 491 - 523 (2014)
Langfellner, J.; Gizon, L.; Birch, A. C.: Time-distance helioseismology: A new averaging scheme for measuring flow vorticity. Astronomy and Astrophysics 570, A90 (2014)
Papini, E.; Gizon, L.; Birch, A. C.: Propagating Linear Waves in Convectively Unstable Stellar Models: a Perturbative Approach. Solar Physics 289, pp. 1919 - 1929 (2014)
Roudier, T.; Švanda, M.; Rieutord, M.; Malherbe, J. M.; Burston, R.; Gizon, L.: Structure and evolution of solar supergranulation using SDO/HMI data. Astronomy and Astrophysics 567, A138 (2014)
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.
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.