Jafarzadeh, S.; Schiavo, L. A. C. A.; Fedun, V.; Solanki, S. K.; Stangalini, M.; Calchetti, D.; Verth, G.; Jess, D. B.; Grant, S. D. T.; Ballai, I.et al.; Gafeira, R.; Keys, P. H.; Fleck, B.; Morton, R. J.; Browning, P. K.; Silva, S. S. A.; Appourchaux, T.; Gandorfer, A.; Gizon, L.; Hirzberger, J.; Kahil, F.; Orozco Suárez, D.; Schou, J.; Strecker, H.; del Toro Iniesta, J. C.; Valori, G.; Volkmer, R.; Woch, J.: Sausage, kink, and fluting magnetohydrodynamic wave modes identified in solar magnetic pores by Solar Orbiter/PHI. Astronomy and Astrophysics 688, p. A2 (2024)
Larson, T. P.; Schou, J.: Correction to: Improved Helioseismic Analysis of Medium-ℓ Data from the Michelson Doppler Imager. Solar Physics 299, p. 61 (2024)
Larson, T. P.; Schou, J.: Correction to: Global-Mode Analysis of Full-Disk Data from the Michelson Doppler Imager and the Helioseismic and Magnetic Imager. Solar Physics 299, p. 62 (2024)
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).