Bučík, R.; Innes, D.; Mason, G. M.; Wiedenbeck, M. E.; Gómez-Herrero, R.; Nitta, N. V.: 3He-rich Solar Energetic Particles in Helical Jets on the Sun. The Astrophysical Journal 852, 76 (2018)
Attie, R.; Innes, D. E.; Solanki, S. K.; Glassmeier, K.-H.: Relationship between supergranulation flows, magnetic cancellation and network flares. Astronomy and Astrophysics 596, A15 (2016)
Bučík, R.; Innes, D. E.; Mason, G. M.; Wiedenbeck, M. E.: Energy spectra of 3He-rich solar energetic particles associated with coronal waves. J. Phys.: Conf. Ser. 767, 012002 (2016)
Bučík, R.; Innes, D. E.; Mason, G. M.; Wiedenbeck, M. E.: Association of 3He-rich solar energetic particles with large-scale coronal waves. Astrophysical Journal 833, 63 (2016)
Innes, D. E.; Bučík, R.; Guo, L.-J.; Nitta, N.: Observations of solar X-ray and EUV jets and their related phenomena. Astron. Nachrichten 337, pp. 1024 - 1032 (2016)
Innes, D. E.; Heinrich, P.; Inhester, B.; Guo, L.-J.: Analysis of UV and EUV emission from impacts on the Sun after 2011 June 7 eruptive flare. Astronomy and Astrophysics 592, A17 (2016)
Kumar, P.; Innes, D. E.; Cho, K.-S.: Flare-Generated Shock Wave Propagation Through Solar Coronal Arcade Loops and an Associated Type II Radio Burst. Astrophysical Journal 828 (1), 28 (2016)
Mason, G. M.; Nitta, N. V.; Wiedenbeck, M. E.; Innes, D. E.: Evidence for a Common Acceleration Mechanism for Enrichments of He-3 And Heavy Ions in Impulsive SEP Events. Astrophysical Journal 823 (2), 138 (2016)
Bučík, R.; Innes, D. E.; Chen, N.-H.; Mason, G. M.; Gomez-Herrero, R.; Wiedenbeck, M. E.: Long-lived energetic particle source regions on the Sun. Journal of Physics: Conference Series 642, 012002 (2015)
Bučík, R.; Innes, D. E.; Guo, L.; Mason, G. M.; Wiedenbeck, M. E.: Observations of EUV waves in 3He-rich solar energetic particle events. Astrophysical Journal 812 (1), 53 (2015)
Chen, N.-H.; Bučík, R.; Innes, D. E.; Mason, G. M.: Case studies of multi-day 3He-rich solar energetic particle periods. Astronomy and Astrophysics 580, A16 (2015)
Innes, D.; Guo, L.; Huang, Y.-M.; Bhattacharjee, A.: IRIS Si IV Line Profiles: An Indication for the Plasmoid Instability During Small-scale Magnetic Reconnection on the Sun. Astrophysical Journal 813, pp. 86 - 96 (2015)
Kumar, P.; Innes, D.: Partial Reflection and Trapping of a Fast-mode Wave in Solar Coronal Arcade Loops. Astrophysical Journal 803, pp. L23 - L29 (2015)
Panesar, N.; Sterling, A.; Innes, D.; Moore, R.: Destabilization of a Solar Prominence/Filament Field System by a Series of Eight Homologous Eruptive Flares Leading to a CME. Astrophysical Journal 811, pp. 5 - 15 (2015)
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.
A collision nearly 30 years ago permanently changed Jupiter's atmospheric chemistry; the aftermath is still helping to better understand the gas giant.
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.