Name: Pencil Code User Meeting 2024
Start: 2024-09-23T09:15:00+00:00
End: 2024-09-27T14:30:00+00:00
Location: ICE

Monday, 23 September
- 09:15 → 10:00
  
  Welcome Coffee and introduction
- 10:00 → 10:40
  
  Pencil Code science output & development since 2023 40m
  
  Speaker: Prof. Axel Brandenburg
- 10:40 → 11:20
  
  MHD models of inner solar corona including solar wind 40m
  
  Speaker: Prof. Piyali Chatterjee
- 11:20 → 12:00
  
  Evolution of Reconnection Flux during Solar Coronal Mass Ejection 40m
  
  Speaker: Dr Samriddhi S Maity
- 12:00 → 12:30
  
  Discussion - coding 30m
- 12:30 → 14:30
  
  lunch break 2h
- 14:30 → 16:00
  
  Coding session: Electromagnetic energy conversion during reheating 1h 30m
  
  Speaker: Prof. Axel Brandenburg
- 16:00 → 16:30
  
  Coffee 30m
- 16:30 → 18:00
  
  Coding session: src/special/disp_current.f90 1h 30m
Tuesday, 24 September
- 09:30 → 10:10
  
  Phase transitions in early universe 40m
  
  Speaker: Dr Alberto Roper Pol
- 10:10 → 10:40
  
  Endpoints of turbulent MHD decay 30m
  
  Speaker: Prof. Axel Brandenburg
- 10:40 → 11:00
  
  Idea for Pencil code extension for planetary simulations 20m
  
  Speaker: Prof. Yasuhito Narita
- 11:00 → 11:30
  
  Coffee break 30m
- 11:30 → 12:30
  
  GPU-accelerated Pencil Code simulations 1h
  
  Speaker: Dr Matthias Reinhardt
- 12:30 → 14:30
  
  lunch break 2h
- 14:30 → 15:00
  
  Discussion - coding 30m
- 15:00 → 16:00
  
  Probing primordial magnetic fields with cosmic microwave background and 21 cm line observations 1h
  
  Observations show magnetic fields to be associated with a great number of objects and on very different scales in the universe, from stars, to galaxies, clusters of galaxies and even beyond.
  It is an open question if there exists a magnetic field on cosmological scales which pervades the whole universe. One possible origin could be in the very early universe.
  Because of contributions to the cosmological perturbations as well as magnetic field dissipation primordial magnetic fields directly influence, for example, the temperature anisotropies and polarization of the cosmic microwave background (CMB) as well as large scale structure.
  New possibilities to constrain primordial magnetic fields arise with current and upcoming observations of the 21 cm line of neutral hydrogen such as with the Square Kilometre Array Observatory (SKAO).
  Using 21 cm intensity maps as well as cross correlations of the CMB Doppler mode and the 21 cm signal prospects of constraining primordial cosmic magnetic fields are considered for LOFAR and SKAO for homogeneous and inhomogeneous reionization. In particular the latter in combination with SKA1-mid shows promising signal-over-noise ratios.
  
  Speaker: Prof. KERSTIN ELENA KUNZE
- 16:00 → 16:30
  
  Coffee break 30m
- 16:30 → 18:00
  
  Discussion - coding 1h 30m
- 20:00 → 22:00
  
  Dinner downtown Barcelona 2h
Wednesday, 25 September
- 09:30 → 10:30
  
  IO modules coding session 1h
  
  Speaker: Prof. Philippe Bourdin
- 10:30 → 11:00
  
  Discussion - coding session (Tutorial) 30m
  
  Speaker: Dr Jennifer Schober
- 11:00 → 11:30
  
  Coffee break 30m
- 11:30 → 12:30
  
  Discussion - coding session (Tutorial) 1h
  
  Speaker: Dr Jennifer Schober
- 12:30 → 14:30
  
  lunch break 2h
- 14:30 → 15:00
  
  Report from the steering committee 30m
- 15:00 → 16:00
  
  Discussion - coding session 1h
- 16:00 → 16:30
  
  Coffee break 30m
- 16:30 → 18:00
  
  Coding session: GPU-accelerated Pencil Code simulations 1h 30m
  
  Speaker: Dr Matthias Reinhardt
  
  GPU-Matthias-Presentation3.pptx
- 18:00 → 20:00
  
  Afterwork drinks 2h
Thursday, 26 September
- 09:30 → 10:20
  
  Coding session: Solar mean-field simulations with the Pencil Code 50m
  
  Speaker: Prof. Axel Brandenburg
- 10:20 → 11:00
  
  3D MHD pulsar wind nebulae. 40m
  
  Speaker: Dr Meyer Dominique
- 11:00 → 11:30
  
  Coffee break 30m
- 11:30 → 12:30
  
  Discussion - coding 1h
- 12:30 → 14:30
  
  lunch break 2h
- 14:30 → 15:10
  
  Magnetohydrodynamic simulations of A-type stars:Rotational scaling of core dynamo cycles 40m
  
  Speaker: Dr Juan Pablo Hidalgo
- 15:10 → 15:40
  
  Adaptive multiphysics simulations coupled in Trixi.jl 30m
  
  Speaker: Dr Simon Candelaresi
- 20:00 → 22:00
  
  Dinner downtown Barcelona 2h
Friday, 27 September
- 09:30 → 11:00
  
  Discussion - coding 1h 30m
- 11:00 → 11:30
  
  Coffee break 30m
- 11:30 → 12:30
  
  Discussion - coding - final remarks 1h
- 12:30 → 14:30
  
  lunch break 2h

Pencil Code User Meeting 2024

ICE

Presentation