Axford, W. I.; McKenzie, J. F.: The origin of high speed solar wind streams. In: Solar Wind Seven (Proc. 3rd COSPAR Colloquium, Goslar, Germany 16-20 September 1991), pp. 1 - 5 (Eds. Marsch, E.; Schwenn, R.). Pergamon Press, Oxford (1992)
Axford, W. I.: The origin of cosmic rays. In: Astrophysical Aspects of the Most Energetic Cosmic Rays (Proc. ICRR International Symposium, Kofu, Japan, 1990), pp. 406 - 420 (Eds. Nagano, M.; Takahara, F.). World Scientific Publ. Comp., Singapore (1991)
Daglis, I. A.; Paschalidis, N. P.; Sarris, E. T.; Axford, W. I.; Kremser, G.; Wilken, B.; Gloeckler, G.: Statistical features of the substorm expansion-phase as observed by the AMPTE/CCE spacecraft. In: Magnetospheric Substorms, pp. 323 - 332 (Eds. Kan, J. R.; Potemra, T. A.; Kokubun, S.; Iijima, T.). American Geophysical Union, Washington, D. C. (1991)
Ip, W.-H.; Axford, W. I.: UHE cosmic ray acceleration at extragalactic radio jets. In: Astrophysical Aspects of the Most Energetic Cosmic Rays (Proc. ICRR International Symposium, Kofu, Japan, 1990), pp. 273 - 280 (Eds. Nagano, M.; Takahara, F.). World Scientific Publ. Comp., Singapore (1991)
Axford, W. I.: Introductory lecture - The heliosphere. In: Physics of the Outer Heliosphere (Proc. 1st COSPAR Colloquium on 'Physics of the Outer Heliosphere', Warszawa, Poland, 1989), pp. 7 - 15 (Eds. Grzedzielski, S.; Page, D. E.). Pergamon Press (1990)
Ip, W.-H.; Axford, W. I.: The plasma. In: Physics and Chemistry of Comets (review chapter), pp. 177 - 233 (Ed. Huebner, W. F.). Springer Verlag, Berlin (1990)
Somogyi, A. J.; Axford, W. I.; Erdös, G.; Ip, W.-H.; Shapiro, V. D.; Shevchenko, V. I.: Particle acceleration in the plasma fields near Comet Halley. In: Comet Halley - Investigations, Results, Interpretations, pp. 203 - 219 (Ed. Mason, J.). Ellis Horwood Ltd., Chichester, U. K. (1990)
Axford, W. I.; Sagdeev, R. Z.: The encounters with comet Halley, March 1986. In: Modern Radio Science (Series of Tutorial and General Lectures at 22th URSI General Assembly, Tel Aviv, 24 August-02 September 1987), pp. 155 - 164 (Ed. Cullen, A. L.). ICSU Press, Paris (1987)
Axford, W. I.: Magnetic field reconnection. In: Magnetic Reconnection in Space and Laboratory Plasmas, pp. 1 - 8 (Eds. Jr., H.; W., E.). American Geophysical Union, Washington, D. C. (1984)
Axford, W. I.: Driven and non-driven reconnection; boundary conditions. In: Magnetic Reconnection in Space and Laboratory Plasmas, pp. 360 - 361 (Eds. Jr., H.; W., E.). American Geophysical Union, Washington, D. C. (1984)
Axford, W. I.: The magnetosphere of Uranus. In: Uranus and the Outer Planets (Proc. of IAU/RAS Colloquium No. 60, Bath, 14-16 April 1981), pp. 125 - 142 (Ed. Hunt, G.). Cambridge Univ. Press (1982)
Ip, W. H.; Axford, W. I.: Theories of physical processes in the cometary comae and ion tails (review). In: Comets, pp. 588 - 634 (Ed. Wilkening, L. L.). The University of Arizona Press, Tucson (1982)
Axford, W. I.: The acceleration of galactic cosmic rays. In: Origin of Cosmic Rays, pp. 339 - 358 (Eds. Setti, G.; Spada, G.; Wolfendale, A. W.). IAU (1981)
Axford, W. I.: The acceleration of cosmic rays by shock waves. In: Annales of the New York Academy of Sciences, pp. 297 - 313 (Eds. Ramaty, R.; Jones, F. C.). The New York Academy of Sciences (1981)
Ip, W.-H.; Axford, W. I.: Physics of the planets and satellites. In: Astronomy and Astrophysics; Methods, Constants, Solar System, pp. 146 - 182 (Eds. Schaifers, K.; Voigt, H. H.). Springer-Verlag, Berlin, Heidelberg, New York (1981)
Axford, W. I.: The three-dimensional structure of the interplanetary medium. In: Study of Travelling Interplanetary Phenomena, pp. 145 - 164 (Eds. Shea; A., M.; others). D. Reidel Publ. Comp., Dordrecht, Holland (1977)
Axford, W. I.: Solar wind and cosmic rays - collection of OHP's of Prof. Sir Ian Axford. In: Proceedings of the Cosmic-Ray Research Section of Nagoya University (Ed. Muraki, Y.). Solar-Terrestrial Environment Laboratory, Nagoya University, Chikusa-ku, Nagoya, Japan (2001)
McKenzie, J. F.; Axford, W. I.: Can gravitational effects damp Alfvén waves? In: Physics of the Solar Corona and Transition Region (Proc. Monterey Workshop, August 1999), pp. 153 - 159 (Eds. Engvold, O.; Harvey, J. W.). Kluwer Academic Publ., Dordrecht (2001)
Die ESA-Mission JUICE soll ab 2030 das Jupitersystem erkunden. Nach Vorbeiflügen an Europa und Callisto wird die Raumsonde erstmals in der Geschichte der Raumfahrt in eine Umlaufbahn um den Mond Ganymed einschwenken.
Das Submillimetre Wave Instrument (SWI) wird die Galileischen Monde, die Chemie, die Meteorologie und die Struktur der mittleren Jupiter-Atmosphäre, sowie atmosphärische und magnetosphärische Kopplungsprozesse untersuchen.
Mars Express ist eine ESA Mission zum Mars. Sie hat eine Nutzlast an Bord, die in der Lage ist, die bisher gründlichste Suche nach flüssigem Wasser, das unerlässlich ist für Leben wie wir es kennen, auf dem roten Planeten durchzuführen.
Ein Überblick über alle Arbeits- und Forschungsgruppen der Abteilung für Planetenwissenschaften: Atmosphären der Planeten, Inneres der Planeten, Kleine Körper und Kometen, Oberflächen der Planeten, Plasmaumgebung der Planeten.