activity
19962013
most citedOn Validating an Astrophysical Simulation Code

220 citations · 837 across the 19 of their papers we have counts for

collaborators

16 papers

astro-ph.SR2013★ 6 cited

Modeling coronal magnetic field using spherical geometry: cases with several active regions

Tilaye Tadesse, T. Wiegelmann, K. Olson +1

The magnetic fields in the solar atmosphere structure the plasma, store free magnetic energy and produce a wide variety of active solar phenomena, like flare and coronal mass eject…

astro-ph.SR2012★ 22 cited

A Comparison Between Nonlinear Force-Free Field and Potential Field Models Using Full-Disk SDO/HMI Magnetogram

Tilaye Tadesse, T. Wiegelmann, B. Inhester +3

Measurements of magnetic fields and electric currents in the pre-eruptive corona are crucial to study solar eruptive phenomena, like flare and coronal mass ejections(CMEs). However…

gr-qc2004★ 50 cited

Evolving a puncture black hole with fixed mesh refinement

Breno Imbiriba, John Baker, Dae-Il Choi +5

We present an algorithm for treating mesh refinement interfaces in numerical relativity. We detail the behavior of the solution near such interfaces located in the strong field reg…

astro-ph2003★ 100 cited

Morphology of Rising Hydrodynamic and Magneto-hydrodynamic Bubbles from Numerical Simulations

K. Robinson, L. J. Dursi, P. M. Ricker +11

Recent Chandra and XMM-Newton observations of galaxy cluster cooling flows have revealed X-ray emission voids of up to 30 kpc in size that have been identified with buoyant, magnet…

astro-ph2003★ 64 cited

On Heavy Element Enrichment in Classical Novae

A. Alexakis, A. C. Calder, A. Heger +10

Many classical nova ejecta are enriched in CNO and Ne. Rosner et al. recently suggested that the enrichment might originate in the resonant interaction between large-scale shear fl…

astro-ph2003★ 25 cited

The Response of Model and Astrophysical Thermonuclear Flames to Curvature and Stretch

L. J. Dursi, M. Zingale, A. C. Calder +11

Critically understanding the `standard candle'-like behavior of Type Ia supernovae requires understanding their explosion mechanism. One family of models for Type Ia Supernovae beg…