Ghosh, A.; Chatterjee, S.; Khan, A. R.; Tripathi, D.; Ramaprakash, A. N.; Banerjee, D.; Chordia, P.; Gandorfer, A. M.; Krivova, N.; Nandy, D.et al.; Rajarshi, C.; Solanki, S. K.; Sriram, S.: The Solar Ultraviolet Imaging Telescope onboard Aditya-L1. Proceedings of the SPIE 9905, 990503 (2016)
Wiegelmann, T.; Solanki, S. K.; Borrero, J. M.; Peter, H.; Barthol, P.; Gandorfer, A.; Martínez Pillet, V.; Schmidt, W.; Knölker, M.: Evolution of the Fine Structure of Magnetic Fields in the Quiet Sun: Observations from Sunrise/IMaX and Extrapolations. Solar Physics 283, pp. 253 - 272 (2013)
Guglielmino, S. L.; Martinez Pillet, V.; Bonet, J. A.; del Toro Iniesta, J. C.; Bellot Rubio, L. R.; Solanki, S. K.; Schmidt, W.; Gandorfer, A.; Barthol, P.; Knoelker, M.: The Frontier Between Small-Scale Bipoles and Ephemeral Regions in the Solar Photosphere: Emergence and Decay of an Intermediate-Scale Bipole Observed with SUNRISE/IMaX. Astrophysical Journal 745 (2), 160 (2012)
Martínez González, M. J.; Asensio Ramos, A.; Manso Sainz, R.; Khomenko, E.; Martínez Pillet, V.; Solanki, S. K.; López Ariste, A.; Schmidt, W.; Barthol, P.; Gandorfer, A.: Unnoticed Magnetic Field Oscillations in the Very Quiet Sun Revealed by Sunrise/IMaX. Astrophysical Journal 730, L37 (2011)
Matthews, S. A.; Williams, D. R.; Klein, K.-L.; Kontar, E. P.; Smith, D. M.; Lagg, A.; Krucker, S.; Hurford, G. J.; Vilmer, N.; MacKinnon, A. L.et al.; Zharkova, V. V.; Fletcher, L.; Hannah, I. G.; Browning, P. K.; Innes, D. E.; Trottet, G.; Foullon, C.; Nakariakov, V. M.; Green, L. M.; Lamoureux, H.; Forsyth, C.; Walton, D. M.; Mathioudakis, M.; Gandorfer, A.; Martinez-Pillet, V.; Limousin, O.; Verwichte, E.; Dalla, S.; Mann, G.; Aurass, H.; Neukirch, T.: Solar Particle Acceleration Radiation and Kinetics (SPARK). Experimental Astronomy 33, pp. 237 - 269 (2011)
Yelles Chaouche, L.; Moreno-Insertis, F.; Martínez Pillet, V.; Wiegelmann, T.; Bonet, J. A.; Knölker, M.; Bellot Rubio, L. R.; del Toro Iniesta, J. C.; Barthol, P.; Gandorfer, A.et al.; Schmidt, W.; Solanki, S. K.: Mesogranulation and the Solar Surface Magnetic Field Distribution. Astrophysical Journal 727, L30 (2011)
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).