Widdel, H. U.; Rose, G.; Borchers, R.: Results of conductivity, ion mobility and ion concentration measurements obtained with a parachutet Gerdien aspiration analyses probe in heights below 70 km. Journal of Atmospheric and Terrestrial Physics 41, pp. 1141 - 1147 (1979)
Widdel, H. U.; Rose, G.; Borchers, R.: Payload BIII - an instrument package for the measurement of conductivity, concentration an mobility of positive and negative ions in the meosphere. J. Geophys. 44, pp. 179 - 188 (1977)
Borchers, R.; Rose, G.; Widdel, H. U.: Ergebnisse von Ionendichte- und Ionenbeweglichkeitsmessungen mit einer Fallschirmsonde im Höhenbereich von 72 bis 39 km. Kleinheubacher Berichte 14, pp. 255 - 262 (1971)
Rose, G.; Widdel, H. U.; Borchers, R.: A mesosphere payload to measure the concentration and mobility of positive and negative ions in the height range between 72 and 40 km. J. Brit. Interpl. Soc. 24, pp. 215 - 231 (1971)
Widdel, H. U.; Rose, G.; Borchers, R.: Results of concentration and mobility measurements of positively and negatively charged particles taken by a rocket-borne parachutet aspiration (Gerdien) probe in the height region from 72 to 39 km. Pageoph 84, pp. 154 - 160 (1971)
Widdel, H. U.; Rose, G.; Borchers, R.: Results of conductivity, ion mobility and ion concentration measurements taken with a parachute Gerdien Kondensor experiment during the winter anomaly campaign. In: COSPAR Space Res., pp. 125 - 127 (Eds. Rycroft, M. J.; Stickland, A. C.). Pergamon Press Oxford (1978)
Rose, G.: Hydrodynamic and electrodynamic measurements. In: The Upper Atmosphere: Data Analysis and Interpretation, pp. 219 - 227 (Eds. Dieminger, W.; Hartmann, G. K.; Leitinger, R.). Springer, Berlin (1996)
Grandal, B.; Rose, G.; Holtat, J.; Måseide, K.; Neske, E.; Ott, W.; Spenner, K.; Trøim, J.; Kopka, H.; Stubbe, P.: Preliminary results from the HERO project: In situ measurements of ionospheric modifications using sounding rockets. In: ESA Conference Proceedings SP-195 on ``Active Experiments in Space'' (Alpbach, Austria, 24-28 May 1983), pp. 75 - 80. (1983)
Kohl, H.; La Hoz, C.; Folkestad, K.; Hansen, T.; Kopka, H.; Rose, G.; Stubbe, P.: The electron and ion spectra of radar returns from the critical height during ionospheric heating experiments. In: ESA Conference Proceedings SP-195 on ``Active Experiments in Space'' (Alpbach, Austria, 24-28 May 1983), pp. 91 - 97. (1983)
Rose, G.; Grandal, B.; Neske, E.; w., O.; Spenner, K.; Trøim, J.; Holtet, J.; Måseide, K.; Kopka, H.; Stubbe, P.: First results of the in situ measurements of the HERO heating campaign. In: ESA Conference Proceedings SP-183 on ``European Rocket and Balloon Programmes'' (Interlaken, Switzerland, 14-15 April 1983), pp. 263 - 267. (1983)
Stubbe, P.; Kopka, H.; Rose, G.: Rocket experiments in conjunction with the ionospheric modification experiment in northern Norway. In: Proc. Esrange Symp., Ajaccio, Korsika 24.-29.4., pp. 107 - 111. ESA Publ. Div., Noordwijk (1978)
Recently new, very sensitive observations of the ExoMars Trace Gas Orbiter (TGO) and its instruments NOMAD (Nadir and Occultation for MArs Discovery) an ACS (Atmospheric Chemistry Suite) became available and initiated a number of interesting scientific questions. Some of them are open PhD projects using the MPS General Circulation Model (MPS-GCM).
The Solar Lower Atmosphere and Magnetism (SLAM) group covers many exciting subjects in solar physics, focussing on the development and testing of highly novel solar instrumentation, reduction and analysis of highest quality solar observations, or improving and developing advanced techniques for the analysis of solar observations.
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
Turbulence plays a very important role in many applications, ranging from geophysics and astrophysics to engineering. In our solar system, turbulence is often driving by thermal effect, rotation, and magnetic field. In this project you will use high-fidelity simulation tools, including direct numerical simulations, data assimilation, and machine learning, to study the physics of turbulence, focusing on convection and dynamos.
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).
Inversion codes are used to aid the detailed interpretation of solar spectro-polarimetric data. This computer code attempts to find the atmospheric structure that produced an observed spectrum by minimizing the difference between the observed spectrum and a Stokes spectrum.