Developments in Large Eddy Simulations for Compressible MHD Turbulence in Space Plasma
Insights into the Small-Scale Solar Dynamo from Ensemble Analysis of Magnetic Features
Comparison of inversion codes for polarized line formation in MHD simulations. Milne-Eddington codes
NICOLE: An Open Source, Massively Parallel Code for Non-LTE Synthesis and Inversion of Spectral Lines and Zeeman-induced Stokes Profiles
NO WEBCAST OR RECORDING WILL BE AVAILABLEEnergy transport by kink waves in the solar atmosphere
NO WEBCAST OR RECORDING WILL BE AVAILABLEA simulation of solar convective dynamo: self-consistent maintenance of the solar differential rotation and emerging flux
NO WEBCAST OR RECORDING WILL BE AVAILABLEOpposite polarity and convective flows in simulated sunspot penumbra: comparison with observations
NO HAO COLLOQUIUM JUNE 11
Stellar evolution beyond the standard picture
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