Innes, D. E.; Cameron, R. H.; Fletcher, L.; Inhester, B.; Solanki, S. K.: Break up of returning plasma after the 7 June 2011 filament eruption by Rayleigh-Taylor instabilities. Astronomy and Astrophysics 540, L10 (2012)
Tian, H.; McIntosh, S. W.; Wang, T.; Ofman, L.; De Pontieu, B.; Innes, D. E.; Peter, H.: Persistent Doppler Shift Oscillations Observed with Hinode/EIS in the Solar Corona: Spectroscopic Signatures of Alfvénic Waves and Recurring Upflows. Astrophysical Journal 759, 144 (2012)
Innes, D. E.; Cameron, R. H.; Solanki, S. K.: EUV Jets, Type III Radio Bursts and Sunspot Waves Investigated Using SDO/AIA Observations. Astronomy and Astrophysics 531, L13 (2011)
Kamio, S.; Curdt, W.; Teriaca, L.; Innes, D. E.: Evolution of microflares associated with bright points in coronal holes and in quiet regions. Astronomy and Astrophysics 529, A21 (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)
Innes, D. E.; McIntosh, S. W.; Pietarila, A.: STEREO quadrature observations of coronal dimming at the onset of mini-CMEs. Astronomy and Astrophysics 517, L7 (2010)
McIntosh, S. W.; Innes, D. E.; De Pontieu, B.; Leamon, R. J.: STEREO observations of quasi-periodically driven high velocity outflows in polar plumes. Astronomy and Astrophysics 510, L2 (2010)
Attie, R.; Innes, D. E.; Potts, H. E.: Evidence of photospheric vortex flows at supergranular junctions observed by FG/SOT (Hinode). Astronomy and Astrophysics 493 (2), pp. L13 - L16 (2009)
Innes, D. E.; Genetelli, A.; Attie, R.; Potts, H. E.: Quiet Sun mini-coronal mass ejections activated by supergranular flows. Astronomy and Astrophysics 495, p. 319 (2009)
Bazarghan, M.; Safari, H.; Innes, D. E.; Karami, E.; Solanki, S. K.: A nanoflare model for active region radiance: application of artificial neural networks. Astronomy and Astrophysics 492, pp. L13 - L16 (2008)
Chen, P. F.; Innes, D. E.; Solanki, S. K.: SOHO/SUMER observations of prominence oscillation before eruption. Astronomy and Astrophysics 484, pp. 487 - 493 (2008)
Innes, D. E.; Attie, R.; Hara, H.; Madjarska, M. S.: EIS/ Hinode Observations of Doppler Flow Seen through the 40-Arcsec Wide-Slit. Solar Physics 252, pp. 283 - 292 (2008)
Madjarska, M. S.; Doyle, J. G.; Innes, D. E.; Curdt, W.: Jets or High-Velocity Flows Revealed in High-Cadence Spectrometer and Imager Co-observations? Astrophysical Journal 670, pp. L57 - L60 (2007)
Wang, T. J.; Innes, D. E.; Qiu, J.: Determination of the coronal magnetic field from hot-loop oscillations observed by SUMER and SXT. Astrophysical Journal 656 (1), pp. 598 - 609 (2007)
Wang, T. J.; Innes, D. E.; Solanki, S. K.: Fe XIX observations of active region brightenings in the corona. Astronomy and Astrophysics 455, pp. 1105 - 1113 (2006)
Bewsher, D.; Innes, D. E.; Parnell, C. E.; Brown, D. S.: Comparison of blinkers and explosive events: A case study. Astronomy and Astrophysics 432, pp. 307 - 317 (2005)
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.