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19962025
most citedA Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953

388 citations · 4.5k across the 94 of their papers we have counts for

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Showing 2015Show all

6 papers · 1 filter

astro-ph.SR2015★ 65 cited

Thresholded Power Law Size Distributions of Instabilities in Astrophysics

Markus J. Aschwanden

Power law-like size distributions are ubiquitous in astrophysical instabilities. There are at least four natural effects that cause deviations from ideal power law size distributio…

astro-ph.SR2015★ 41 cited

Benchmark Test of Differential Emission Measure Codes and Multi-Thermal Energies in Solar Active Regions

M. J. Aschwanden, P. Boerner, A. Caspi +3

We compare the ability of 11 Differential Emission Measure (DEM) forward-fitting and inversion methods to constrain the properties of active regions and solar flares by simulating…

nlin.AO2015★ 43 cited

25 Years of Self-Organized Criticality: Numerical Detection Methods

R. T. James McAteer, Markus J. Aschwanden, Michaila Dimitropoulou +5

The detection and characterization of self-organized criticality (SOC), in both real and simulated data, has undergone many significant revisions over the past 25 years. The explos…

astro-ph.SR2015★ 16 cited

Blind Stereoscopy of the Coronal Magnetic Field

Markus J. Aschwanden, Carolus J. Schrijver, Anna Malanushenko

We test the feasibility of 3D coronal-loop tracing in stereoscopic EUV image pairs, with the ultimate goal of enabling efficient 3D reconstruction of the coronal magnetic field tha…

astro-ph.SR2015★ 22 cited

Magnetic Energy Dissipation during the 2014 March 29 Solar Flares

Markus J. Aschwanden

We calculated the time evolution of the free magnetic energy during the 2014-Mar-29 flare (SOL2014-03-29T17:48), the first X-class flare detected by IRIS. The free energy was calcu…

astro-ph.SR2015★ 85 cited

Global Energetics of Solar Flares: II. Thermal Energies

M. J. Aschwanden, P. Boerner, D. Ryan +3

We present the second part of a project on the global energetics of solar flares and CMEs that includes about 400 M- and X-class flares observed with AIA/SDO during the first 3.5 y…