Photospheric Shear Flows along the Magnetic Neutral Line of Active Region 10486 prior to an X10 Flare
Authors:
- Guo YangGYGuo Yang
- Yan XuYXYan Xu
- Wenda CaoWCWenda Cao
- Haimin WangHWHaimin Wang
- Carsten DenkerCDCarsten Denker
- Thomas R. RimmeleTRThomas R. Rimmele
- 11 November 2004
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 617 (2) , L151-L154
Abstract
No abstract availableThis publication has 15 references indexed in Scilit:
- Fast photospheric flows and magnetic fields in a flaring active regionAstronomy & Astrophysics, 2003
- Solar adaptive optics: a progress report2003
- The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI)Solar Physics, 2002
- Observational Determination of the Rate of Magnetic Helicity Transport through the Solar Surface via the Horizontal Motion of Field Line FootpointsThe Astrophysical Journal, 2001
- Near Real-Time Image ReconstructionSolar Physics, 2001
- A Twisted Flux Rope Model for Coronal Mass Ejections and Two-Ribbon FlaresThe Astrophysical Journal, 2000
- The Solar Oscillations Investigation - Michelson Doppler ImagerSolar Physics, 1995
- Precise proper-motion measurement of solar granulationThe Astrophysical Journal, 1988
- A study of the magnetic and velocity fields in an active regionSolar Physics, 1976
- Relationship between some photospheric motions and the evolution of active centersSolar Physics, 1973