Name: CN5 - Turbulence Day
Start: 2023-10-31T11:00:00+01:00
End: 2023-10-31T17:00:00+01:00
Location: MPA

CN5 - Turbulence Day

Tuesday, 31 October 2023 - 11:00

Monday, 30 October 2023
Tuesday, 31 October 2023
11:00 Review 1: Turbulence in the ISM - Max Gronke (MPA)
Review 1: Turbulence in the ISM
- Max Gronke (MPA)
11:00 - 11:30
Room: Lecture Hall E.0.11
11:30 Multiphase gas in a Turbulent medium, with a pinch of magnetic fields - Hitesh Das
Multiphase gas in a Turbulent medium, with a pinch of magnetic fields
- Hitesh Das
11:30 - 11:50
Room: Lecture Hall E.0.11
11:50 The role of physical viscosity in hydrodynamical instabilities - Tirso Marin
The role of physical viscosity in hydrodynamical instabilities
- Tirso Marin
11:50 - 12:10
Room: Lecture Hall E.0.11
12:10 Magnetic fields and the launching of jets in core-collapse supernovae - Martin Obergaulinger
Magnetic fields and the launching of jets in core-collapse supernovae
- Martin Obergaulinger
12:10 - 12:30
Room: Lecture Hall E.0.11
12:30 Lunch Break
Lunch Break
12:30 - 14:00
14:00 Review 2: Turbulent magnetic fields - dissipation, dynamos, and cascades - Axel Brandenburg
Review 2: Turbulent magnetic fields - dissipation, dynamos, and cascades
- Axel Brandenburg
14:00 - 14:30
Room: Lecture Hall E.0.11
14:30 Magnetic bubbles: buoyancy instability at high wave numbers - Gustavo Guerrero
Magnetic bubbles: buoyancy instability at high wave numbers
- Gustavo Guerrero
14:30 - 14:50
Room: Lecture Hall E.0.11
14:50 Formation of protostars and their accretion disks in turbulent magnetized cloud cores - Alexander Mayer
Formation of protostars and their accretion disks in turbulent magnetized cloud cores
- Alexander Mayer
14:50 - 15:10
Room: Lecture Hall E.0.11
15:10 Coffee Break
Coffee Break
15:10 - 15:40
Room: Lecture Hall E.0.11
15:40 Sub- and supersonic turbulence with Discontinuous Galerkin on GPUs - Miha Cernetic
Sub- and supersonic turbulence with Discontinuous Galerkin on GPUs
- Miha Cernetic
15:40 - 16:00
Room: Lecture Hall E.0.11
16:00 Turbulence in Galaxy Clusters with Meshless Finite Mass: Impact of the Hydrodynamical Scheme - Frederick Groth (USM, LMU)
Turbulence in Galaxy Clusters with Meshless Finite Mass: Impact of the Hydrodynamical Scheme
- Frederick Groth (USM, LMU)
16:00 - 16:20
Room: Lecture Hall E.0.11
16:20 Turbulence as a source of Radio Mega Halos - Ludwig Böss (Ludwig-Maximilian Universität (Universitätssternwarte München))
Turbulence as a source of Radio Mega Halos
- Ludwig Böss (Ludwig-Maximilian Universität (Universitätssternwarte München))
16:20 - 16:40
Room: Lecture Hall E.0.11

Choose timezone