S3 Seminars: Archive

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.
Room: Lecture Hall

S3 Seminar: Multiple line inversions of Swedish Solar Telescope spectra (S. Saranathan)

S3 Seminar: Thermal Vacuum/Thermal Balance test of Solar Orbiter PHI flight model (G. Fernandez)

S3 Seminar: The Seismic Structures of Solar-Type Stars: Surmising the Speeds of Sound Inside 16 Cygni (E. Bellinger)

S3 Seminar: Simulations of starspots (M. Panja)

S3 Seminar: Solving the forward problem in helioseismology for an average supergranule(R. Z. Ferret)

S3 Seminar: Deep focusing in time-distance helioseismology (M. Pourabdian)

S3 Seminar: Helioseismic holography (D. Yang)

S3 Seminar: Multiple scattering of acoustic waves (P.-L. Poulier)

S3 Seminar: Stellar activity in low mass stars (E. Johnson)

S3 Seminar: Counter-Evershed flows in sunspots penumbrae (A. Siu)

S3 Seminar: Temperature and velocity in the coma of 67P / CG from MIRO (D. Marshall)

S3 Seminar: How old are red-giant stars in clusters? (N. Themeßl)

S3 Seminar: The search for Europa plume signatures in Galileo particle detectro data (H. Huybrighs)

S3 Seminar: Comet formation in collapsing pebble clouds (S. Lorek)

S3 Seminar: Measuring Mercury´s tides (R. Thor)

S3 Seminar: Layerings in cometary nuclei (B.-K. R.)

S3 Seminar: From axisymmetric to non.axisymmetric: how rotation influences dynamo modes (M.Viviani)

S3 Seminar: Non-axisymmetric structure of the Sun´s toroidal magnetic field (D. Martin Belda)

S3 Seminar: Observations and simulations of the Sun´s polar regions (H. Waller)

S3 Seminar: Local helioseismology and Local Correlation Tracking applied to SDO / HMI observations (B. Proxauf)

S3 Seminar: Noise modeling for exoplanet transits (K. Rodenbeck)

S3 Seminar: Pulsed magnetopause reconnection as a trigger for pulsations in Saturn´s magnetosphere (B. Palmaerts)

S3 Seminar: Brightness of solar magnetic elements as a function of magnetic flux at high spatial resolution (F. Kahil)

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