Seminare am MPS

Zu allen Seminaren und Vorträgen am MPS sind interessierte Besucher herzlich willkommen. Die Präsentationen werden hauptsächlich in englischer Sprache gehalten, genauere Informationen zu Themen, Rednern und Terminen sind auf den einzelnen Seminar-Seiten zu finden. Bei Institutsseminaren und Kolloquien präsentieren geladene Gastwissenschaftler anderer Institute Erfolge und Resultate ihrer Forschung. In den S3 Seminaren erklären Doktoranden der Internationalen Max Planck Research School (IMPRS) ihre Arbeit. In den Seminaren über Planeten und Kometen (PGS) sowie den Seminaren über die Sonne und sonnenähnlicher Sterne (SSGS), berichten die Wissenschaftler aus den jeweiligen Abteilungen über neueste Ergebnisse und Fortschritte in ihren Projekten und stellen neue Missionen vor. Bei allen Seminaren findet im Anschluss an den Vortrag eine kurze Diskussions- bzw. Fragerunde zum Thema statt.
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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ESPOS: Wave Period Variability in a Quiescent Solar Prominence (Aneta Wiśniewska)

ESPOS
On 26 September 2022, we observed a quiescent solar prominence with Hα imaging spectroscopy using the Solar Dynamics Doppler Imager (SDDI) on the SMART telescope. Unlike earlier works that detected 4- and 15-min oscillations through long-slit, 1D wavelet methods, we adapt the wavelet analysis to 3D data to explore the full prominence structure. Complementary data from SDO/AIA (304 Å, 171 Å) STEREO-A/EUVI (304 Å), and Solar Orbiter EUI/FSI (304 Å, 174 Å) enable a multi-view, multi-thermal investigation of wave periodicity across the prominence. Our aim is to characterize how oscillatory periods are distributed in plasma at different temperatures and viewing angles, thereby assessing wave propagation and variability throughout the prominence body. [mehr]
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.

PGS: 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 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.

PGS: TBA (Rody Erftemeijer)

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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.

PGS: TBA (Vignesh Vaikundaraman)

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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.

PGS: TBA (Illya Lohay)

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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: reliability 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 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.

PGS: TBA (Miles Lindner)

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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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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.

PGS: TBA (Fiona Speller)

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