activity
20172019
most citedGeneration mechanisms of quasi-parallel and quasi-circular flare ribbons in a confined flare

32 citations · 80 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.SR20198 cited

A Hot Cusp-Shaped Confined Solar Flare

Aaron Hernandez-Perez, Yang Su, Julia K. Thalmann +5

We analyze a confined flare that developed a hot cusp-like structure high in the corona (H ~ 66 Mm). A growing cusp-shaped flare arcade is a typical feature in the standard model o…

astro-ph.SR201921 cited

Pre-eruption processes: heating, particle acceleration and the formation of a hot channel before the 2012 October 20 M9.0 limb flare

Aaron Hernandez-Perez, Yang Su, Astrid M. Veronig +3

We report a detailed study of the pre-eruption activities that led to the occurrence of an M9.0 flare/CME event on 2012 October 20 in NOAA AR 11598. This includes the study of the…

astro-ph.SR2018

Numerical Simulation of Coronal Waves Interacting with Coronal Holes: III. Dependence on Initial Amplitude of the Incoming Wave

Isabell Piantschitsch, Bojan Vrsnak, Arnold Hanslmeier +4

We performed 2.5D magnetohydrodynamic (MHD) simulations showing the propagation of fast-mode MHD waves of different initial amplitudes and their interaction with a coronal hole (CH…

astro-ph.SR2018

Numerical Simulation of Coronal Waves Interacting with Coronal Holes: II. Dependence on Alfvén Speed Inside the Coronal Hole

Isabell Piantschitsch, Bojan Vrsnak, Arnold Hanslmeier +4

We used our newly developed magnetohydrodynamic (MHD) code to perform 2.5D simulations of a fast-mode MHD wave interacting with coronal holes (CH) of varying Alfvén speed which res…

astro-ph.SR2018

Numerical Simulation of Coronal Waves interacting with Coronal Holes: I. Basic Features

Isabell Piantschitsch, Bojan Vrsnak, Arnold Hanslmeier +5

We developed a new numerical code that is able to perform 2.5D simulations of a magnetohydrodynamic (MHD) wave propagation in the corona, and its interaction with a low density reg…

astro-ph.SR201732 cited

Generation mechanisms of quasi-parallel and quasi-circular flare ribbons in a confined flare

Aaron Hernandez-Perez, Julia K. Thalmann, Astrid M. Veronig +3

We analyze a confined multiple-ribbon M2.1 flare (SOL2015-01-29T11:42) that originated from a fan-spine coronal magnetic field configuration, within active region NOAA 12268. The o…