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)
A star’s chemical composition strongly influences the ultraviolet radiation it emits into space and thus the conditions for the emergence of life in its neighbourhood.
A single star has provided information about the collision of the Milky Way with the dwarf galaxy Gaia-Enceladus. The event likely took place approximately 11.5 billion years ago.