Axford, W. I.; McKenzie, J. F.: Implications of observations of the solar wind and corona for solar wind models. Astrophysics and Space Science 243, pp. 1 - 3 (1996)
Daglis, I. A.; Axford, W. I.: Fast ionospheric response to enhanced activity in geospace: Ion feeding of the inner magnetotail. Journal Geophysical Research 101, pp. 5047 - 5065 (1996)
Daglis, I. A.; Axford, W. I.; Livi, S.; Wilken, B.; Grande, M.; Søraas, F.: Auroral ionospheric ion feeding of the inner plasma sheet during substorms. J. Geomag. Geoelectr. 48, pp. 729 - 739 (1996)
Hovestadt, D.; Hilchenbach, M.; Bürgi, A.; Klecker, B.; Laeverenz, P.; Scholer, M.; Grünwaldt, H.; Axford, W. I.; Livi, S.; Marsch, E.et al.; Wilken, B.; Winterhoff, H. P.; Ipavich, F. M.; Bedini, P.; Coplan, M. A.; Galvin, A. B.; Gloeckler, G.; Bochsler, P.; Balsiger, H.; Fischer, J.; Geiss, J.; Kallenbach, R.; Wurz, P.; Reiche, K.-U.; Gliem, F.; Judge, D. L.; Ogawa, H. S.; Hsieh, K. C.; Möbius, E.; Lee, M. A.; Managadze, G. G.; Verigin, M. I.; Neugebauer, M.: CELIAS-Charge, element and isotope analysis system for SOHO. Solar Physics 162, pp. 441 - 481 (1995)
Nielsen, E.; Axford, W. I.; Hagfors, T.; Kopka, H.; Armand, N. A.; Andrianov, V. A.; Shtern, D. J.; Breus, T.: The ``Long Wavelength Radar'' on the Mars-94 Orbiter. Advances in Space Research 15, pp. (4)163 - (4)178 (1995)
Ratkiewicz, R.; Axford, W. I.; McKenzie, J. F.: Similarity solutions for synchrotron emission from a supernova blast wave. Astronomy and Astrophysics 291, pp. 935 - 942 (1994)
Dougherty, M. K.; Krymskii, A. M.; Breus, T. K.; Southwood, D. J.; Axford, W. I.: The electromagnetic effects of the solar wind interaction with Phobos. Advances in Space Research 13, pp. (10)295 - (10)298 (1993)
Krymskii, A. M.; Breus, T. K.; Dougherty, M. K.; Southwood, D. J.; Axford, W. I.: The electromagnetic effects of the solar wind interaction with the Phobos neutral gas halo and dust torus. Planetary and Space Science 40, pp. 1033 - 1041 (1992)
McKenzie, J. F.; Ershkovich, A. I.; Axford, W. I.: Stability of a cometary ionosphere/ionopause including pressure effects. Astrophysical Journal 360, pp. 275 - 278 (1990)
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.
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.