Showing 1–20 of 21 results
/ Date/ Name
Apr 9, 2015Spectropolarimetrically accurate magnetohydrostatic sunspot model for forward modelling in helioseismologyAug 27, 2025Structure and dynamics of the internetwork solar chromosphere: results of a small-scale dynamo simulationApr 6, 2022Chromospheric Extension of the MURaM CodeMay 31, 2022Small-scale Dynamo in Cool Stars: I. Changes in stratification and near-surface convection for main-sequence spectral typesOct 9, 2023Testing MURaM and MPS-ATLAS against the quiet solar spectrumJul 11, 2024Magnetograms underestimate even unipolar magnetic flux nearly everywhere on the solar diskAug 6, 2025Probing chromospheric fine structures with a Hα proxy using MURaM-ChEApr 30, 2026Self-consistent numerical simulations for the formation and dynamics of solar prominencesApr 22, 2021Transient small-scale brightenings in the quiet solar corona: a model for campfires observed with Solar OrbiterDec 4, 20153D simulations of realistic power halos in magneto-hydrostatic sunspot atmospheres: linking theory and observationNov 17, 2024Investigating explosive events in a 3D quiet-Sun model: Transition region and coronal responseDec 15, 2025Statistical properties of spicules in MURaM-ChEJul 16, 2021Refactoring the MPS/University of Chicago Radiative MHD(MURaM) Model for GPU/CPU Performance Portability Using OpenACC DirectivesJun 19, 2025Coriolis force acting on near-surface horizontal flows during simulations of flux emergence produces a tilt angle consistent with Joy's law on the SunSep 15, 2025Magnetic reconnection sustains the mass budget of the solar windDec 25, 2025A self-consistent 3D MHD model producing a solar blowout jetJan 6, 2015MHD wave refraction and the acoustic halo effect around solar active regions - a 3D studyNov 16, 2025Simulations of structured upflows from plumes and their connection to the solar windMar 9, 2022Doppler shifts of spectral lines formed in the solar transition region and coronaFeb 10, 2025Sunrise III: Overview of Observatory and Instruments