PENUMBRAL FINE STRUCTURE AND DRIVING MECHANISMS OF LARGE-SCALE FLOWS IN SIMULATED SUNSPOTS
Open Access
- 3 February 2011
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 729 (1)
- https://doi.org/10.1088/0004-637x/729/1/5
Abstract
No abstract availableThis publication has 64 references indexed in Scilit:
- SEARCHING FOR OVERTURNING CONVECTION IN PENUMBRAL FILAMENTS: SLIT SPECTROSCOPY AT 0.″2 RESOLUTIONThe Astrophysical Journal, 2010
- The velocity field of sunspot penumbraeAstronomy & Astrophysics, 2009
- Evidence of convective rolls in a sunspot penumbraAstronomy & Astrophysics, 2008
- Convection and the Origin of Evershed Flows in Sunspot PenumbraeThe Astrophysical Journal, 2008
- Twisting Motions of Sunspot Penumbral FilamentsScience, 2007
- Temporal evolution of the Evershed flow in sunspotsAstronomy & Astrophysics, 2007
- Magnetostatic penumbra models with field-free gapsAstronomy & Astrophysics, 2006
- Dark cores in sunspot penumbral filamentsNature, 2002
- Cold, Supersonic Evershed Downflows in a SunspotThe Astrophysical Journal, 2001
- A Dynamical Model for the Penumbral Fine Structure and the Evershed Effect in SunspotsThe Astrophysical Journal, 1998