Logo: IMPRS for Solar System Science at the University of Göttingen and at TU Braunschweig - International Max Planck Research School - Solar System School

S3 Seminars

PhD students of the International Max Planck Research School present their work in the IMPRS S3 seminars. Every Wednesday during term, two doctorate students present their methods, progress, and results in a short talk of about half an hour. Questions may be asked after the talk.
A rocky celestial body in blue hues in front of a dark blue background. The body's shape is spherical, and it is surrounded by much smaller, also spherically-shaped bodies. The scene's vicinity has a nebular quality to it, which is partially illuminated by a bright light on the top right.

Simulations of the Helium distribution in Mercury's plasma environment (Fabio Prencipe)

Planetary Group Seminar
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A Sun drawn in comic style with an active surface, with ten rays of various lengths emerging from its disk forming a spiked wheel shape that supports colorful planets as well as a comet and a cloud of pebbles positioned at its various end points.

Tools talks

S3 Seminar
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A rocky celestial body in blue hues in front of a dark blue background. The body's shape is spherical, and it is surrounded by much smaller, also spherically-shaped bodies. The scene's vicinity has a nebular quality to it, which is partially illuminated by a bright light on the top right.

Modeling Ganymede’s Surface Charging Processes (Betty Pei-Chun Tsai)

Planetary Group Seminar
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A Sun drawn in comic style with an active surface, with ten rays of various lengths emerging from its disk forming a spiked wheel shape that supports colorful planets as well as a comet and a cloud of pebbles positioned at its various end points.

Real-time onboard processing for the Photospheric Magnetic Field Imager (PMI) onboard ESA's Vigil mission (Deepa Muraleedharan)

S3 Seminar
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A Sun drawn in comic style with an active surface, with ten rays of various lengths emerging from its disk forming a spiked wheel shape that supports colorful planets as well as a comet and a cloud of pebbles positioned at its various end points.

Stereoscopic disambiguation of solar vector magnetograms: reliablity evaluations, and comparison with single-view disambiguation (Xiang Li)

S3 Seminar
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A Sun drawn in comic style with an active surface, with ten rays of various lengths emerging from its disk forming a spiked wheel shape that supports colorful planets as well as a comet and a cloud of pebbles positioned at its various end points.

Chromospheric Fe I lines in the near-ultraviolet solar spectrum: Simulations and observations (Edvarda Harnes)

S3 Seminar
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A Sun drawn in comic style with an active surface, with ten rays of various lengths emerging from its disk forming a spiked wheel shape that supports colorful planets as well as a comet and a cloud of pebbles positioned at its various end points.

Investigating high-speed outflows from a coronal hole with UV spectroscopy (Mario Roco Moraleda)

S3 Seminar
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A Sun drawn in comic style with an active surface, with ten rays of various lengths emerging from its disk forming a spiked wheel shape that supports colorful planets as well as a comet and a cloud of pebbles positioned at its various end points.

Reconstruction of the annual solar irradiance over the past 9 millennia (Duresa Temaj)

S3 Seminar
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A Sun drawn in comic style with an active surface, with ten rays of various lengths emerging from its disk forming a spiked wheel shape that supports colorful planets as well as a comet and a cloud of pebbles positioned at its various end points.

Turbulence in Keplerian flow (Abhiroop Bhadra)

S3 Seminar
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