Solar MHD 2022
Advances in Solar MHD Numerical Simulations in the Era of High-
Resolution Observations, Solar MHD 2022 (UKUS 6)
7-10 August 2022, Eastbourne, UK
The meeting covered a number of topics related to the analysis of data obtained in solar MHD simulations and their interpretation in connection to high spatial and temporal resolution observations. In particular, the following topics were covered:
• Simulating excitation and propagation of MHD waves in solar plasma,
• Simulating plasma instabilities,
• Effective numerical tools towards more realistic physics in modelling,
• Numerical simulations and spectral line synthesis,
• Identification and analysis of plasma flows.
Selected Talks
Two-fluid implementation in MPI-AMRVAC with
applications to the solar chromosphere
Beatrice Popescu Braileanu
COCONUT: a fast converging coronal MHD model
M. Brchnelova
Multi3D: a 3D non-LTE polarized radiative transfer code
Flavio Calvo
MBP merger, an alternative solar/stellar coronal heating mechanism
Hidetaka Kuniyoshi
Radiative MHD simulation of the solar corona with RAMENS
Haruhisa Iijima
Formation of prominences with fine structure
Veronika Jercic
MPI-AMRVAC: open-source grid-adaptive simulations
Rony Keppens
Corrugation instability in partially ionised slow-mode shocks
Ben Snow
Detection and dynamics of small scale vortex flows in the solar atmosphere
Kostas Tziotziou
Ensemble simulations from Solar magnetograms to 1 A.U.
Tony Arber
Mode identification of Magnetohydrodynamic (MHD) waves in simulated solar atmosphere
Nitin Yadav