388 citations · 4.5k across the 94 of their papers we have counts for
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Nonlinear Force-Free Magnetic Field Fitting to Coronal Loops with and without Stereoscopy
Markus J. Aschwanden
We developed a new nonlinear force-free magnetic field (NLFFF) forward-fitting algorithm based on an analytical approximation of force-free and divergence-free NLFFF solutions, whi…
A Nonlinear Force-Free Magnetic Field Approximation Suitable for Fast Forward-Fitting to Coronal Loops. III. The Free Energy
Markus J. Aschwanden
An analytical approximation of a nonlinear force-free magnetic field (NLFFF) solution was developed in Paper I, while a numerical code that performs fast forward-fitting of this NL…
The Spatio-Temporal Evolution of Solar Flares Observed with AIA/SDO: Fractal Diffusion, Sub-Diffusion, or Logistic Growth ?
Markus J. Aschwanden
We explore the spatio-temporal evolution of solar flares by fitting a radial expansion model that consists of an exponentially growing acceleration phase, followed by a dece…
Self-Organized Criticality Systems in Astrophysics (Chapter 13)
Markus J. Aschwanden
Chapter 13: SOC Systems in Astrophysics --- Content list: 13.1 Theory -- 13.1.1 The Sacle-Free Probability Theorem - 13.1.2 The Fractal-Diffusive Spatio-Temporal Relationship - 13.…
First 3D Reconstructions of Coronal Loops with the STEREO A+B Spacecraft: IV. Magnetic Modeling with Twisted Force-Free Fields
Markus J. Aschwanden, Jean-Pierre Wuelser, Nariaki V. Nitta +3
The three-dimensional (3D) coordinates of stereoscopically triangulated loops provide strong constraints for magnetic field models of active regions in the solar corona. Here we us…
Solar Stereoscopy with STEREO/EUVI A and B spacecraft from small (6 deg) to large (170 deg) spacecraft separation angles
Markus J. Aschwanden, Jean-Pierre Wülser, Nariaki Nitta +1
We performed for the first time stereoscopic triangulation of coronal loops in active regions over the entire range of spacecraft separation angles ($α_{sep}\approx 6^\circ, 43^\ci…