Grensing, D.; Marsch, E.; Steeb, W.-H.: Magnetic and electric properties of the Hubbard model for the f.c.c. Lattice. Physical Review B 17, pp. 2221 - 2232 (1978)
Marsch, E.; Steeb, W.-H.; Grensing, D.: One-Dimensional Hubbard Model With Nearest and Second Nearest Neighbour Hopping in the Hartree-Fock Approximation. J. Phys. F: Metal Phys. 7, pp. 401 - 406 (1977)
Rosenbauer, H.; Schwenn, R.; Marsch, E.; Meyer, B.; Miggenrieder, H.; Montgomery, M.; Mühlhäuser, K.-H.; Pilipp, W.; Voges, W.; Zink, S. K.: A Survey on Initial Results of the Helios Plasma Experiment. J. Geophys. 42, pp. 561 - 580 (1977)
Marsch, E.: Force-force correlation function method for the ideal resistance of the Hubbard model. J. Phys. C: Solid State Phys. 9, pp. L117 - L120 (1976)
Steeb, W.-H.; Marsch, E.: Thermodynamics of a two-point doubly degenerate Hubbard model in the half-filled case. Phys. Stat. Sol. (b) 78, pp. K39 - K44 (1976)
Steeb, W.-H.; Marsch, E.: A new upper bound for the free energy of the Hubbard model based on the cluster approach. Phys. Stat. Sol. (b) 69, pp. K149 - K152 (1975)
Solanki, S. K.; Marsch, E.: Solar Space Missions: present and future. In: Formation and Evolution of Cosmic Structures: Reviews in Modern Astronomy, Volume 21, pp. 229 - 248 (Ed. Röser, S.). Wiley-VCH, Weinheim (2009)
Marsch, E.: Waves and turbulence in the solar corona. In: The Sun and the Heliosphere as an Integrated System, pp. 283 - 317 (Eds. Poletto, G.; Suess, S. T.). Kluwer Academic Publishers, Dordrecht, The Netherlands (2004)
Marsch, E.; Axford, W. I.; McKenzie, J. F.: Solar Wind. In: The Dynamic Sun, pp. 374 - 402 (Ed. Dwivedi, B.). Cambridge University Press, Cambridge (2003)
Marsch, E.: Solar Wind: Kinetic Properties. In: Encyclopedia of Astronomy and Astrophysics, pp. 2862 - 2866 (Ed. Murdin, P.). Institut of Physics Publishing, Nature Publishing Group (2001)
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.