PhD thesis projects assigned to students

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). more

Understanding the formation and evolution of planets from micron-sized dust grains to fully-formed planets more

Experimental petrology or geochemistry more

A Bepi Colombo Mission to Mercury project (DLR funding) more

Part time researcher / graduate student position in Cometary Science at TU Braunschweig in Prof. Agarwal’s group, deadline 18 September 2024, see https://www.tu-braunschweig.de/en/igep/job-posting more

Cosmochemical investigations on the heritage of volatiles in Earth, Mars, and the Moon more

Numerical simulations to better understand the complete reversals of the geodynamo dipole more

The Sun’s planets and small objects have undergone substantial evolution. Deciphering the history of our cosmic home is not a simple task even though we now have access to a multitude of data gathered by space missions, remote observations, and laboratory studies of diverse samples. A significant fraction of materials available for the study of planetary bodies come from meteorites. more

Numerical simulations to explore how minor bodies like asteroids, comets and KBOs formed more

Statistically analyse the large set of grain coma data in Rosetta/OSIRIS images of comet 67P/C-G more

Development of various analysis tools, processing pipelines, and data enhancement procedures for ESA's upcoming space weather mission more

(Solar-C) more

Spectroscopic and imaging data from observations and synthesized from 3D MHD models of the Solar corona more

Putting stellar superflares from SUIT/Aditya-1 data on the same scale as the solar flares more

Solar irradiance variability as seen by Mars general circulation models and comparison to HOPE data more

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The solar magnetic field is mostly axisymmetric at large-scale with latitudinal dynamo wave propagating from mid-latitudes towards the equator, as can be seen from observations of the solar cycle. Reproducing this pattern is one of the main demands that a numerical model has to satisfy. more

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Assigned PhD project: PLATO PhD position at CNES (Paris) and MPSSR (Göttingen): application deadline 22 March 2021 more

Solar irradiance variability as seen by Mars general circulation models and comparison to HOPE data more

Establishing a new method to detect extra-solar planets more