Goesmann, F.; Brinckerhoff, W. B.; Raulin, F.; Goetz, W.; Danell, R. M.; Getty, S. A.; Siljestrom, S.; Mißbach, H.; Steininger, H.; Arevalo Jr., R. D.et al.; Buch, A.; Freissinet, C.; Grubisic, A.; Meierhenrich, U. J.; Pinnick, V. T.; Stalport, F.; Szopa, C.; Vago, J. L.; Lindner, R.; Schulte, M. D.; Brucato, J. R.; Glavin, D. P.; Grand, N.; Li, X.; van Amerom, F. H. W.; The Moma Science Team: The Mars Organic Molecule Analyzer (MOMA) Instrument: Characterization of Organic Material in Martian Sediments. Astrobiology 17 (6-7), pp. 655 - 685 (2017)
Giri, C.; McKay, C. P.; Goesmann, F.; Schäfer, N.; Li, X.; Steininger, H.; Brinckerhoff, W. B.; Gautier, T.; Reitner, J.; Meierhenrich, U. J.: Carbonization in Titan Tholins: implication for low albedo on surfaces of Centaurs and trans-Neptunian objects. Int. J. Astrobiology 15 (3), pp. 231 - 238 (2016)
Giri, C.; Goesmann, F.; Steele, A.; Gautier, T.; Steininger, H.; Krüger, H.; Meierhenrich, U. J.: Competence evaluation of COSAC flight spare model mass spectrometer: In preparation of arrival of Philae lander on comet 67P/ChuryumovGerasimenko. Planetary and Space Science 106, pp. 132 - 141 (2015)
Li, X.; Danell, R. M.; Brinckerhoff, W. B.; Pinnick, V. T.; van Amerom, F.; Arevalo, R. D.; Getty, S. A.; Mahaffy, P. R.; Steininger, H.; Goesmann, F.: Detection of Trace Organics in Mars Analog Samples Containing Perchlorate by Laser Desorption/Ionization Mass Spectrometry. Astrobiology 15, pp. 104 - 110 (2015)
Goesmann, F.; Raulin, F.; Bredehoeft, J. H.; Cabane, M.; Ehrenfreund, P.; MacDermott, A. J.; McKenna-Lawlor, S.; Meierhenrich, U. J.; Munoz Caro, G. M.; Szopa, C.et al.; Sternberg, R.; Roll, R.; Thiemann, W. H.-P.; Ulamec, S.: COSAC prepares for sampling and in situ analysis of cometary matter from comet 67P/Churyumov-Gerasimenko. Planetary and Space Science 103, pp. 318 - 330 (2014)
Szopa, C.; Sternberg, R.; Coscia, D.; Goesmann, F.; Gomes, R.; Legrand, S.; Jerome, M.; Meierhenrich, U. J.; Raulin, F.: Gas chromatography for in situ analysis of a cometary nucleus V. Study of capillary columns' robustness submitted to long-term reduced environmental pressure conditions. J. Chromatogr. A 1368, pp. 211 - 216 (2014)
Bishop, J. L.; Franz, H. B.; Goetz, W.; Blake, D. F.; Freissinet, C.; Steininger, H.; Goesmann, F.; Brinckerhoff, W. B.; Getty, S.; Pinnick, V. T.et al.; Mahaffy, P. R.; Darby, D. M.: Coordinated analyses of Antarctic sediments as Mars analog materials using reflectance spectroscopy and current flight-like instruments for CheMin, SAM and MOMA. Icarus 224 (2), pp. 309 - 325 (2013)
Meierhenrich, U. J.; Cason, J. R. L.; Szopa, C.; Sternberg, R.; Raulin, F.; Thiemann, W. H.-P.; Goesmann, F.: Evaluating the robustness of the enantioselective stationary phases on the Rosetta mission against space vacuum vaporization. Advances in Space Research 52 (12), pp. 2080 - 2084 (2013)
Evans, A.; Meinert, C.; Giri, C.; Goesmann, F.; Meierhenrich, U.: Chirality, photochemistry and the detection of amino acids in interstellar ice analogues and comets. Chemical Society Reviews 41, pp. 5447 - 5458 (2012)
Goesmann, F.; McKenna-Lawlor, S.; Roll, R.; Bredehöft, J. H.; Meierhenrich, U.; Raulin, F.; Thiemann, W.; Caro, G. M. M.; Szopa, C.: Interpretation of COSAC mass spectrometer data acquired during Rosettas Lutetia fly-by 10 July 2010. Planetary and Space Science 66, pp. 187 - 191 (2012)
Morse, A. D.; Altwegg, K.; Andrews, D. J.; Auster, H. U.; Carr, C. M.; Galand, M.; Goesmann, F.; Gulkis, S.; Lee, S.; Richter, I.et al.; Sheridan, S.; Stern, S. A.; AHearn, M. F.; Feldman, P.; Parker, J.; Retherford, K. D.; Weaver, H. A.; Wright, I. P.: The Rosetta campaign to detect an exosphere at Lutetia. Planetary and Space Science 66, pp. 165 - 172 (2012)
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).
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.
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.
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.