activity
20082026
most citedSolar surface emerging flux regions: a comparative study of radiative MHD modeling and Hinode SOT observations

177 citations · 534 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

Probing the Physics of the Solar Corona with High-Resolution Observations using SKA-Mid

Mark C. M. Cheung, John S. Morgan, Rohit Sharma +3

We examine the capability of the SKA-Mid telescope for probing solar coronal structure and evolution. Using radiative magnetohydrodynamics simulations of a solar flare, we synthesi…

astro-ph.SR2015★ 29 cited

Magnetic Jam in the Corona of the Sun

F. Chen, H. Peter, S. Bingert +1

The outer solar atmosphere, the corona, contains plasma at temperatures of more than a million K, more than 100 times hotter that solar surface. How this gas is heated is a fundame…

astro-ph.SR2014★ 134 cited

High-resolution Observations of the Shock Wave Behavior for Sunspot Oscillations with the Interface Region Imaging Spectrograph

H. Tian, E. DeLuca, K. K. Reeves +20

We present the first results of sunspot oscillations from observations by the Interface Region Imaging Spectrograph. The strongly nonlinear oscillation is identified in both the sl…

astro-ph.SR2014★ 56 cited

A model for the formation of the active region corona driven by magnetic flux emergence

F. Chen, H. Peter, S. Bingert +1

We present the first model that couples the formation of the corona of a solar active region to a model of the emergence of a sunspot pair. This allows us to study when, where, and…

astro-ph.SR2014★ 138 cited

Numerical simulations of active region scale flux emergence: From spot formation to decay

M. Rempel, M. C. M Cheung

We present numerical simulations of active region scale flux emergence covering a time span of up to 6 days. Flux emergence is driven by a bottom boundary condition that advects a…

astro-ph2008★ 177 cited

Solar surface emerging flux regions: a comparative study of radiative MHD modeling and Hinode SOT observations

M. C. M. Cheung, M. Schuessler, T. D. Tarbell +1

We present results from numerical modeling of emerging flux regions on the solar surface. The modeling was carried out by means of 3D radiative MHD simulations of the rise of buoya…