Chilson, P. B.; Palmer, R. D.; Muschinski, A.; Hooper, D. A.; Schmidt, G.; Steinhagen, H.: SOMARE-99: A demonstrational field campaign for ultrahigh-resolution VHF atmospheric profiling using frequency diversity. Radio Science 36 (4), pp. 695 - 707 (2001)
Muschinski, A.; Chilson, P. B.; Palmer, R. D.; Hooper, D. A.; Schmidt, G.; Steinhagen, H.: Boundary-layer convection and diurnal variation of vertical-velocity characteristics in the free troposphere. Quarterly Journal Royal Meteorological Society 127, pp. 423 - 443 (2001)
Palmer, R. D.; Chilson, P. B.; Muschinski, A.; Schmidt, G.; Yu, T.-Y.; Steinhagen, H.: SOMARE-99: Observations of tropospheric scattering layers using multiple-frequency range imaging. Radio Science 36 (4), pp. 681 - 693 (2001)
Muschinski, A.; Chilson, P. B.; Kern, S.; Nielinger, J.; Schmidt, G.; Prenosil, T.: First frequency-domain interferometry observation of large-scale vertical motion in the atmosphere. Journal of the Atmospheric Sciences 56, pp. 1248 - 1259 (1999)
Chilson, P. B.; Muschinski, A.; Schmidt, G.: First observations of Kelvin-Helmholtz billows in an upper level jet stream using VHF frequency domain interferometry. Radio Science 32, pp. 1149 - 1160 (1997)
Kilburn, C. A. D.; Kinglsey, S.; Quegan, S.; Rüster, R.; Schmidt, G.: Super-resolution: a new technique for MST radar studies of atmospheric thin layers. Journal of Atmospheric and Terrestrial Physics 57, pp. 1135 - 1151 (1995)
Steinhagen, H.; Christoph, A.; Czechowsky, P.; Görsdorf, U.; Gube-Lenhardt, M.; Lippmann, J.; Neisser, J.; Rüster, R.; Schmidt, G.; Wergen, W.et al.; Yoe, J. G.: Field campaign for the comparison of SOUSY radar wind measurements with rawinsonde and model data. Annales Geophysicae 12 (8), pp. 746 - 764 (1994)
Yoe, J. G.; Czechowsky, P.; Rüster, R.; Schmidt, G.: Spatial variability of the aspect sensitivity of VHF radar echoes in the troposphere and lower stratosphere during jet stream passages. Annales Geophysicae 12 (8), pp. 733 - 745 (1994)
Inhester, B.; Ulwick, J. C.; Cho, J.; Kelley, M. C.; Schmidt, G.: Consistency of rocket and radar electron density observations: implication about the anisotropy of mesospheric turbulence. Journal of Atmospheric and Terrestrial Physics 52, pp. 855 - 873 (1990)
Lübken, F. J.; von Zahn, U.; Manson, A.; Rüster, R.; Schmidt, G.; Widdel, H. U.: Mean state densities, temperatures and winds during the MAC/SINE and MAC/EPSILON campaign. Journal of Atmospheric and Terrestrial Physics 52, pp. 955 - 970 (1990)
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).
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.
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.
The MPS is one of the leading institutes worldwide in building instruments for solar research, both for ground based observatories as well as for balloon and space-borne missions. Scientists and engineers of MPS conceive new observing methods and develop novel instruments of highest technological complexity. These instruments are built in house, tested, calibrated, and used at the best solar observatories in the world, or delivered to NASA and ESA to be launched to space.
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.