activity
20072025
most citedA Model for the Sources of the Slow Solar Wind

325 citations · 1.7k across the 34 of their papers we have counts for

collaborators

34 papers

physics.space-ph2025

Ion Charge States from a Global Time-Dependent Wave-Turbulence-Driven Model of the Solar Wind: Comparison with in-situ Measurements

Pete Riley, Roberto Lionello, Yeimy J. Rivera

Solar wind charge-state measurements contain a wealth of knowledge related to the properties of the solar corona from where they originated. However, their interpretation has remai…

astro-ph.SR2023

Solar Eruptions Triggered by Flux Emergence Below or Near a Coronal Flux Rope

T. Török, M. G. Linton, J. E. Leake +4

Observations have shown a clear association of filament/prominence eruptions with the emergence of magnetic flux in or near filament channels. Magnetohydrodynamic (MHD) simulations…

astro-ph.SR2023

CORHEL-CME: An Interactive Tool For Modeling Solar Eruptions

Jon Linker, Tibor Torok, Cooper Downs +5

Coronal Mass Ejections (CMEs) are immense eruptions of plasma and magnetic fields that are propelled outward from the Sun, sometimes with velocities greater than 2000 km/s. They ar…

astro-ph.SR2023

Deflection of Coronal Mass Ejections in Unipolar Ambient Magnetic Fields

Michal Ben-Nun, Tibor Török, Erika Palmerio +5

The trajectories of coronal mass ejections (CMEs) are often seen to substantially deviate from a purely radial propagation direction. Such deviations occur predominantly in the cor…

astro-ph.SR2023

Time-Dependent Dynamics of the Corona

Emily I. Mason, Roberto Lionello, Cooper Downs +2

We present in this Letter the first global comparison between traditional line-tied steady state magnetohydrodynamic models and a new, fully time-dependent thermodynamic magnetohyd…

astro-ph.SR2023

Global MHD Simulations of the Time-Dependent Corona

Roberto Lionello, Cooper Downs, Emily I. Mason +5

We describe, test, and apply a technique to incorporate full-sun, surface flux evolution into an MHD model of the global solar corona. Requiring only maps of the evolving surface f…