High-resolution proper motions in a sunspot penumbra
Abstract
Local correlation tracking techniques are used to measure proper motions in a series of high angular resolution (~0.1 arcsec) penumbra images. If these motions trace true plasma motions, then we have detected converging flows that arrange the plasma in long narrow filaments co-spatial with dark penumbral filaments. Assuming that these flows are stationary, the vertical stratification of the atmosphere and the conservation of mass suggest downflows in the filaments of the order of 200 m/s. The association between downflows and dark features may be a sign of convection, as it happens with the non-magnetic granulation. Insufficient spatial resolution may explain why the estimated vertical velocities are not fast enough to supply the radiative losses of penumbrae.
Keywords
Cite
@article{arxiv.astro-ph/0510220,
title = {High-resolution proper motions in a sunspot penumbra},
author = {I. Marquez and J. Sanchez Almeida and J. A. Bonet},
journal= {arXiv preprint arXiv:astro-ph/0510220},
year = {2009}
}
Comments
To appear in ApJ. 11 pages with 9 figures. Movie at http://www.iac.es/proyect/solarhr/pencork.html