2016/09/22 by N. Magyar, T. Van Doorsselaere
Biochemistry, Genetics and Molecular Biology · Physics and Astronomy · #Amplitude #Coronal loop #Geomagnetism and Paleomagnetism Studies #Instability #Ionosphere and magnetosphere dynamics #Kink instability #Loop (graph theory) #Mode (computer interface) #Nonlinear system #Oscillation (cell signaling) #Solar and Space Plasma Dynamics #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/201629010
published as A&A 595, A81 (2016) · 10 pages, 8 figures
arxiv created 2016/09/22 · openalex publication_date 2016/10/03 · openalex created_date 2016/10/07 · arxiv updated 2016/11/02 · openalex updated_date 2026/08/05
Aims. We aim to study the standing fundamental kink mode of coronal loops in the nonlinear regime, investigating the changes in energy evolution in the cross-section and oscillation amplitude of the loop which are related to nonlinear effects, in particular to the development of the Kelvin-Helmholtz instability (KHI).