Contributed by Avijeet Prasad. Posted on July 29, 2022
Inverse Evershed flow is derived from chromospheric observations. Coupling these flow with the non force-free model, the authors find that the flow is driven along magnetic field lines connecting network elements with the outer penumbra by a gas pressure difference.
Contributed by Johannes Löhner-Böttcher. Posted on May 28, 2014
The statistical analysis of flow fields in and around sunspots indicates a distinct nature of the moat and Evershed flows.