Harra, L.; Andretta, V.; Appourchaux, T.; Baudin, F.; Bellot-Rubio, L.; Birch, A.; Boumier, P.; Cameron, R. H.; Carlsson, M.; Corbard, T.et al.; Davies, J.; Fazakerley, A.; Fineschi, S.; Finsterle, W.; Gizon, L.; Harrison, R.; Hassler, D.M.; Leibacher, J.; Liewer, P.; Macdonald, M.; Maksimovic, M.; Murphy, N.; Naletto, G.; Nigro, G.; Owen, C.; Martínez-Pillet, V.; Rochus, P.; Romoli, M.; Sekii, T.; Spadaro, D.; Veronig, A.; Schmutz, W.: A journey of exploration to the polar regions of a star: probing the solar poles and the heliosphere from high helio-latitude. Experimental Astronomy (2021)
Panja, M.; Cameron, R. H.; Solanki, S. K.: Sunspot Simulations: Penumbra Formation and the Fluting Instability. The Astrophysical Journal 907 (2), 102 (2021)
Yadav, N.; Cameron, R. H.; Solanki, S. K.: Vortex flow properties in simulations of solar plage region: Evidence for their role in chromospheric heating. Astronomy and Astrophysics 645, A3 (2021)
Yadav, N.; Cameron, R. H.; Solanki, S. K.: Slow magneto-acoustic waves in simulations of a solar plage region carry enough energy to heat the chromosphere. Astronomy and Astrophysics 652, A43 (2021)
Yadav, N.; Cameron, R. H.; Solanki, S. K.: Simulations Show that Vortex Flows Could Heat the Chromosphere in Solar Plage. Astrophysical Journal, Letters 894 (2), L17 (2020)
Cameron, R. H.; Jiang, J.: The relationship between flux emergence and subsurface toroidal magnetic flux. Astronomy and Astrophysics; EDP Sciences, Les Ulis Cedex A France 631, A27 (2019)
Cameron, R. H.; Schüssler, M.: Solar activity: periodicities beyond 11 years are consistent with random forcing. Astronomy and Astrophysics 625, A28 (2019)
Nielsen, M. B.; Gizon, L.; Cameron, R. H.; Miesch, M.: Starspot rotation rates versus activity cycle phase: Butterfly diagrams of Kepler stars are unlike that of the Sun. Astronomy and Astrophysics 622, A85 (2019)
Boro Saikia, S.; Marvin, C. J.; Jeffers, S. V.; Reiners, A.; Cameron, R. H.; Marsden, S. C.; Petit, P.; Warnecke, J.; Yadav, A. P.: Chromospheric activity catalogue of 4454 cool stars: Questioning the active branch of stellar activity cycles. Astronomy and Astrophysics 616, A108 (2018)
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).