PhD thesis projects offered

All partner institutes in the Solar System School (Institute for Astrophysics, Institute for Geophysics, and Max Planck Institute for Solar System Research) may offer and support PhD projects in the Solar System School. The PhD topics are as diverse as the research fields of the participating partner institutions. The topics include all areas of our own Solar system (the Sun and its planets and minor bodies), embedded in the wider geo- and astrophysical context, and extend to other stars and their planetary systems. Correspondingly, the following disciplines in geo- and astrophysics are represented in the Solar System School: Earth and planetary sciences, Solar and stellar physics, helioseismology, asteroseismology, and to some extent extra-solar planets. Since the methods of research comprise instrumentation development, calibration and improvement , ground- and space-based observations, remote-sensing or in-situ measurements in space exploration missions, data analysis and interpretation, numerical simulations and theoretical modeling, some projects may additionally require good skills in programming, in mathematics, or in engineering.

The following list gives an overview of the variety of research topics, but is not necessarily complete. Further projects may yet become available: This list still is updated from time to time. Please check the list again before submitting your application. Applications may be submitted between 1 October and 1 November.

Open PhD Projects

The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections. more

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. more

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. more

Study time series of solar active regions with sequences of magneto-hydro-static equilibria more

Hydrodynamic simulations of near surface convection and waves in the Sun and stars more

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. more

For PhD students whose project is already funded and who are applying for admission to the IMPRS, or for applicants who want to bring their own funding and their own project idea to the IMPRS. more

Getting to the truth about the solar chromosphere more

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