A Comprehensive Radiative Magnetohydrodynamics Simulation of Active Region Scale Flux Emergence from the Convection Zone to the Corona

A comprehensive three-dimensional radiative magnetohydrodynamic simulation of a solar flare

A low upper limit on the subsurface rise speed of solar active regions ⬇️

scientific article

Characterization of magneto-convection in sunspots

Comparing Radiative Transfer Codes and Opacity Samplings for Solar Irradiance Reconstructions

Convolutional Neural Networks and Stokes Response Functions

Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code

Effects of Spectral Resolution on Simple Magnetic Field Diagnostics of the Mg ii H and K Lines

Efficient Numerical Treatment of Ambipolar and Hall Drift as Hyperbolic System

scientific article published in 2021

Eruption of a Magnetic Flux Rope in a Comprehensive Radiative Magnetohydrodynamic Simulation of Flare-productive Active Regions

Heating of the solar chromosphere through current dissipation

Limitations and Biases in the Retrieval of the Polar Magnetic Field. I. The Role of the Magnetic Filling Factor in Milne–Eddington Inversions of Simulated Hinode/SP Data

Measuring the Magnetic Origins of Solar Flares, Coronal Mass Ejections, and Space Weather

scientific article

On the Contribution of Quiet-Sun Magnetism to Solar Irradiance Variations: Constraints on Quiet-Sun Variability and Grand-minimum Scenarios

Penumbral structure and outflows in simulated sunspots

scientific article published in Science

Probing the Physics of the Solar Atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal Heating

scientific article published in 'The Astrophysical Journal' in February 2022

Probing the Physics of the Solar Atmosphere with the Multi-slit Solar Explorer (MUSE). II. Flares and Eruptions

Rapid blue- and redshifted excursions in H α line profiles synthesized from realistic 3D magnetohydrodynamic simulations

Robust climate responses to extreme solar minimum forcing and their hemispheric differences

preprint posted 28 January 2022

Small-Scale Dynamos: From Idealized Models to Solar and Stellar Applications

Small-scale Dynamo Simulations: Magnetic Field Amplification in Exploding Granules and the Role of Deep and Shallow Recirculation

Small-scale loops heated to transition region temperatures and their chromospheric signatures in the simulated solar atmosphere

Superstrong photospheric magnetic fields in sunspot penumbrae

The Coronal Veil

The Dimmest State of the Sun

scientific article published in 2020

The Solar Photospheric Continuum Brightness as a Function of Mean Magnetic Flux Density. I. The Role of the Magnetic Structure Size Distribution

Transport of Internetwork Magnetic Flux Elements in the Solar Photosphere

Using the Butterfly Effect to Probe How the Sun Generates Acoustic Noise

What the Sudden Death of Solar Cycles Can Tell Us About the Nature of the Solar Interior