Cavalié, T.; Billebaud, F.; Dobrijevic, M.; Fouchet, T.; Lellouch, E.; Encrenaz, T.; Brillet, J.; Moriarty-Schieven, G. H.; Wouterloot, J. G. A.; Hartogh, P.: First observation of CO at 345 GHz in the atmosphere of Saturn with the JCMT. New constraints on its origin. Icarus 203, pp. 531 - 540 (2009)
Cavalié, T.; Moreno, R.; Lellouch, E.; Hartogh, P.; Jarchow, C.; Venot, O.; Hersant, F.; Selsis, F.; Orton, G.; Encrenaz, T.et al.; Fletcher, L.: First submillimeter observation of CO in the stratosphere of Uranus with Herschel-HIFI. European Planetary Science Congress, London, UK (2015)
Cavalié, T.; Hue, V.; Hartogh, P.; Lellouch, E.; Cassidy, T.; Dobrijevic, M.; Jarchow, C.; Moreno, R.: Is Enceladus Saturn's source of water? European Planetary Science Congress , Cascais, Portugal (2014)
Cavalié, T.; Venot, O.; Selsis, F.; Hersant, F.; Hartogh, P.: The Deep O/H Ratio in Uranus and Neptune from CO Spectroscopy and Thermochemical Modeling. Workshop on the Study of the Ice Giant Planets, Laurel, Maryland, USA (2014)
Orton, G.; Fletcher, L. N.; Feuchtgruber, H.; Lellouch, E.; Moreno, R.; Encrenaz, T.; Hartogh, P.; Jarchow, C.; Swinyard, B.; Cavalié, T.et al.; Moses, J.; Burgdorf, M.; Hammel, H.; Line, M.; Mainzer, A. K.; Hofstadter, M.; Sandell, G. H.; Dowell, C. D.; Pantin, E.; Fujiyoshi, T.: Models for Temperature and Composition in Uranus from Spitzer, Herschel and Ground-Based Infrared through Millimeter Observations. American Astronomical Society, DPS meeting #46, Tucson, AZ, USA (2014)
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).