Rose, G.: Die H- und E-Wellenfeldexperimente des Heating-Raketenprogramms. Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany (1980)
Rose, G.: A survey of experimental E-region data obtained between 1967 and 1975. Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany (1976)
Schlegel, K.; Rose, G.; Widdel, H. U.: Interplanetary magnetic field polarity changes and D-region radio wave absorption. Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany (1976)
Widdel, H. U.; Rose, G.; Borchers, R.: Experimental results on the variation of ion condctivity and mobility in the mesosphere. Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany (1976)
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).