Pencil Code User Meeting 2024

UTC
ICE

ICE

Albert Elias-López (Institue of Space Sciences), Fabio Del Sordo (ICE), Felipe Navarrete
Description


Presentation


The 2024 Pencil Code User Meeting will be held in ICE from Monday 23rd to Friday 27th of September. The Institute of Space Sciences (ICE-CSIC / IEEC) is a scientific and technological research institution with contributions to many areas in astronomy, instrumentation, astrophysics, cosmology, gravitation and engineering.

Note that ICE is located in the campus of Universitat Autonoma de Barcelona (UAB), which is NOT in Barcelona City, but within the metro area. It and can be reached easily with public transport in about 40 minutes from downtown Barcelona. For convenience, we advise to choose the accommodation within the campus hotel (Exe Campus Hotel, Cerdanyola del Vallès), which is about 10-15 walking distance.

 

Participants
  • Alberto Roper Pol
  • Antonino Salvino Midiri
  • Axel Brandenburg
  • AZEEZ OLUWAGBENGA OSENI
  • Clara Dehman
  • Deepen Garg
  • Dominique Meyer
  • Fabio Del Sordo
  • Felipe Navarrete
  • Frederick Gent
  • Gustav Larsson
  • Hongzhe Zhou
  • Isabella Kraus
  • Jennifer Schober
  • Juan Pablo Hidalgo
  • Kerstin Kunze
  • Kishore Gopalakrishnan
  • Luis Mauricio Villarroel Casanova
  • Madeline Salomé
  • Matthias Rheinhardt
  • Matías Liempi
  • MAYUSREE DAS
  • Murman Gurgenidze
  • Naveen Jingade
  • Nishant Singh
  • Oksana Iarygina
  • Petri Käpylä
  • Philippe Bourdin
  • Piyali Chatterjee
  • Ramkishor Sharma
  • Samriddhi S Maity
  • Simon Candelaresi
  • Sovan Sau
  • SUBHASIS MAITI
  • Thomas Celora
  • Toma Oregel-Chaumont
  • Yasin Qazi
  • Yasuhito Narita
    • 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
    • 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
    • 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
    • 18:00 20:00
      Afterwork drinks 2h
    • 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
    • 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
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