Chen, Y.-T.; Lin, H. W.; Holman, M. J.; Payne, M. J.; Fraser, W. C.; Lacerda, P.; Ip, W.-H.; Chen, W.-P.; Kudritzki, R.-P.; Jedicke, R.et al.; Wainscoat, R. J.; Tonry, J. L.; Magnier, E. A.; Waters, C.; Kaiser, N.; Wang, S.-Y.; Lehner, M.: Discovery of a New Retrograde Trans-Neptunian Object: Hint of a Common Orbital Plane for Low Semimajor Axis, High-Inclination TNOs and Centaurs. Astrophysical Journal 827 (2), L24 (2016)
Lorek, S.; Gundlach, B.; Lacerda, P.; Blum, J.: Comet formation in collapsing pebble clouds. What cometary bulk density implies for the cloud mass and dust-to-ice ratio. Astronomy and Astrophysics 587, A128 (2016)
Muntean, E. A.; Lacerda, P.; Field, T. A.; Fitzsimmons, A.; Fraser, W. C.; Hunniford, A. C.; McCullough, R. W.: A laboratory study of water ice erosion by low-energy ions. Mon. Not. Roy. Astron. Soc. 462 (3), pp. 3361 - 3367 (2016)
Pfalzner, S.; Davies, M. B.; Gounelle, M.; Johansen, A.; Muenker, C.; Lacerda, P.; Zwart, S. P.; Testi, L.; Trieloff, M.; Veras, D.: The formation of the solar system. Physica Scripta 90 (6), 068001 (2015)
Hsieh, H. H.; Denneau, L.; Fitzimmons, A.; Hainaut, O. R.; Ishiguro, M.; Jedicke, R.; Kaluna, H. M.; Keane, J. V.; Kleyna, J.; Lacerda, P.et al.; MacLennan, E. M.; Meech, K. J.; Moskovitz, N. A.; Riesen, T.; Schunova, E.; Snodgrass, C.; Trujillo, C. A.; Urban, L.; Veres, P.; Wainscoat, R. J.; Yang, B.: Search for the Return of Activity in Active Asteroid 176P/Linear. Astronomical Journal 147 (4), 89 (2014)
Lorek, S.; Lacerda, P.; Gundlach, B.; Blum, J.: Compaction of ice pebbles in collapsing pebble clouds and the dust-to-ice ratio of comets. European Planetary Science Congress 2015, Nantes, France (2015)
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.
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.
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.
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).