no code implementations • 1 Feb 2021 • Ryan J. Campbell, Mihalis Mathioudakis, Manuel Collados, Peter H. Keys, Andrés Asensio Ramos, Chris J. Nelson, David Kuridze, Aaron Reid
We present three regions of interest (ROIs), tracking the dynamics of small scale magnetic features.
Solar and Stellar Astrophysics
1 code implementation • 9 Apr 2018 • Jiajia Liu, Chris J. Nelson, Robert Erdélyi
Comparisons between swirls detected in Bifrost numerical MHD simulations and both ground-based and space-borne observations, suggest that: 1) the spatial resolution of data plays a vital role in the total number and radii of swirls detected; and 2) noise introduced by seeing effects could decrease the detection rate of swirls, but has no significant influences in determining their inferred properties.
Solar and Stellar Astrophysics
