Bhatia, T. S.; Cameron, R.; Peter, H.; Solanki, S.: Small-scale dynamo in cool stars. III. Changes in the photospheres of F3V to M0V stars. Astronomy and Astrophysics 681, p. A32 (2024)
Breu, C. A.; Peter, H.; Solanki, S. K.; Cameron, R.; De Moortel, I.: Non-thermal broadening of coronal lines in a 3D MHD loop model. Monthly Notices of the Royal Astronomical Society (2024)
Breu, C.; Peter, H.; Solanki, S. K.; Cameron, R.; De Moortel, I.: Non-thermal broadening of coronal lines in a 3D MHD loop model. Monthly Notices of the Royal Astronomical Society 530, pp. 2361 - 2377 (2024)
Chen, Y.; Mandal, S.; Peter, H.; Chitta, L. P.: Bidirectional propagating brightenings in arch filament systems observed by Solar Orbiter/EUI. Astronomy and Astrophysics 692, p. A119 (2024)
Chitta, L. P.; Zhukov, A. N.; Berghmans, D.; Peter, H.; Parenti, S.; Mandal, S.; Aznar Cuadrado, R.; Schühle, U.; Teriaca, L.; Auchère, F.et al.; Barczynski, K.; Buchlin, É.; Harra, L.; Kraaikamp, E.; Long, D. M.; Rodriguez, L.; Schwanitz, C.; Smith, P. J.; Verbeeck, C.; Seaton, D. B.: Picoflare jets power the solar wind emerging from a coronal hole on the Sun. Science 38, pp. 867 - 872 (2023)
Baker, D.; Démoulin, P.; Yardley, S. L.; Mihailescu, T.; van Driel-Gesztelyi, L.; D'Amicis, R.; Long, D. M.; To, A. S. H.; Owen, C. J.; Horbury, T. S.et al.; Brooks, D. H.; Perrone, D.; French, R. J.; James, A. W.; Janvier, M.; Matthews, S.; Stangalini, M.; Valori, G.; Smith, P.; Aznar Cuadrado, R.; Peter, H.; Schühle, U.; Harra, L.; Barczynski, K.; Berghmans, D.; Zhukov, A. N.; Rodriguez, L.; Verbeeck, C.: Observational Evidence of S-web Source of the Slow Solar Wind. The Astrophysical Journal 950, p. 65 (2023)
Cheng, X.; Xing, C.; Aulanier, G.; Solanki, S. K.; Peter, H.; Ding, M. D.: Deciphering the Slow-rise Precursor of a Major Coronal Mass Ejection. The Astrophysical Journal 954, p. L47 (2023)
Li, Z.; Cheng, X.; Ding, M. D.; Chitta, L. P.; Peter, H.; Berghmans, D.; Smith, P. J.; Auchère, F.; Parenti, S.; Barczynski, K.et al.; Harra, L.; Schühle, U.; Buchlin, É.; Verbeeck, C.; Aznar Cuadrado, R.; Zhukov, A. N.; Long, D. M.; Teriaca, L.; Rodriguez, L.: Evidence of external reconnection between an erupting mini-filament and ambient loops observed by Solar Orbiter/EUI. Astronomy and Astrophysics 673, p. A83 (2023)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
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).