Mall, U.; Wöhler, C.; Grumpe, A.; Bugiolacchi, R.; Bhatt, M.: Characterization of lunar soils through spectral features extraction in the NIR. Advances in Space Research 54 (10), pp. 2029 - 2040 (2014)
Wöhler, C.; Grumpe, A.; Berezhnoy, A.; Bhatt, M. U.; Mall, U.: Integrated topographic, photometric and spectral analysis of the lunar surface: Application to impact melt flows and ponds. Icarus 235, pp. 86 - 122 (2014)
Bugiolacchi, R.; Mall, U.; Bhatt, M.; McKenna-Lawlor, S.; Ullaland, K.: From the Imbrium Basin to crater Tycho: The first regional spectral distribution map derived from SIR-2 near-infrared data. Icarus 223, pp. 804 - 818 (2013)
Reddy, V.; Le Corre, L.; O'Brien, D. P.; Nathues, A.; Cloutis, E. A.; Durda, D. D.; Bottke, W. F.; Bhatt, M. U.; Nesvorny, D.; Buczkowski, D.et al.; Scully, J. E. C.; Palmer, E. M.; Sierks, H.; Mann, P. J.; Becker, K. J.; Beck, A. W.; Mittlefehldt, D.; Li, J.-Y.; Gaskell, R.; Russell, C. T.; Gaffey, M. J.; McSween, H. Y.; McCord, T. B.; Combe, J.-P.; Blewett, D.: Corrigendum to ``Delivery of dark material to Vesta via carbonaceous chondritic impacts'' [Icarus 221, pg 544, 2012]. Icarus 223 (1), p. 632 - 632 (2013)
Bhatt, M.; Mall, U.; Bugiolacchi, R.; McKenna-Lawlor, S.; Banaszkiewicz, M.; Nathues, A.; Ullaland, K.: Lunar iron abundance determination using the 2-μm absorption band parameters. Icarus 220 (1), pp. 51 - 64 (2012)
Bugiolacchi, R.; Mall, U.; Bhatt, M.: NIR spectral investigation of the Delisle/Diophantus crater region by the SIR-2 instrument. In: Proceedings of the 42nd Lunar and Planetary Science Conference. (2011)
Bhatt, M. U.: Mineralogical analysis and iron abundance estimation of the Moon using the SIR-2 and other VIS-NIR spectrometers on-board the lunar orbiter Chandrayaan-1. Dissertation, Technische Universität Clausthal (2012)
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.