Ning, Z.; Innes, D. E.; Solanki, S. K.: Line profile characteristics of solar explosive event bursts. Astronomy and Astrophysics 419, pp. 1141 - 1148 (2004)
Innes, D. E.; McKenzie, D. E.; Wang, T.: Observations of 1000 km s−1 Doppler shift in 107 K solar flare supra-arcade. Solar Physics 217, pp. 267 - 279 (2003)
Landi, E.; Feldman, U.; Innes, D.; Curdt, W.: Mass motions and plasma properties in the 107 K flare solar corona. Astrophysical Journal 582, pp. 506 - 519 (2003)
Innes, D. E.: Coordinated observations of the quiet Sun transition region using SUMER spectra, TRACE images and MDI magnetograms. Astronomy and Astrophysics 378, pp. 1067 - 1077 (2001)
Torsti, J.; Kocharov, L.; Innes, D. E.; Laivola, J.; Sahla, T.: Injection of energetic protons during solar eruption on 1999 May 9: Effect of flare and coronal mass ejection. Astronomy and Astrophysics 365, pp. 198 - 203 (2001)
Brooks, D. H.; Fischbacher, G. A.; Fludra, A.; Harrison, R. A.; Innes, D. E.; Landi, E.; Landini, M.; Lang, J.; Lanzafame, A. C.; Loch, S. D.et al.; McWhirter, R. W. P.; Summers, H. P.: A study of opacity in SOHO-SUMER and SOHO-CDS spectral observations. I. Opacity deduction at the limb. Astronomy and Astrophysics 357, pp. 697 - 715 (2000)
Brooks, D. H.; Fischbacher, G. A.; Fludra, A.; Harrison, R. A.; Innes, D. E.; Landi, E.; Landini, M.; Lang, J.; Lanzafame, A. C.; Loch, S. D.et al.; McWhirter, R. W. P.; Summers, H. P.; Thompson, W. T.: The quiet Sun extreme ultraviolet spectrum observed in normal incidence by the SOHO coronal diagnostic spectrometer. Astronomy and Astrophysics 347, pp. 277 - 312 (1999)
Harrison, R. A.; Lang, J.; Brooks, D. H.; Innes, D. E.: A study of extreme ultraviolet blinker activity. Astronomy and Astrophysics 351, pp. 1115 - 1132 (1999)
Innes, D. E.; Inhester, B.; Srivastava, N.; Brekke, P.; Harrison, R. A.; Matthews, S. A.; Noëns, J. C.; Schmieder, B.; Thompson, B. J.: Multi-wavelength observations of the onset phase of a coronal mass ejection. Solar Physics 186, pp. 337 - 361 (1999)
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.