Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
10695009 | Advances in Space Research | 2005 | 4 Pages |
Abstract
An active region filament was well observed on September 4, 2002 with THEMIS at the Teide observatory and SOHO/MDI. The full Stokes parameters of the filament were obtained in Hα and FeI 6302 Ã
lines. Using the data, we have studied the fine structure of the filament and obtained the parameters at the barb endpoints, including intensity, velocity and longitudinal magnetic field. Our results indicate: (a) the Doppler velocities are quiet different at barb endpoints; (b) the longitudinal magnetic fields at the barb endpoints are very weak; (c) there is a strong magnetic field structure under the filament spine.
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Space and Planetary Science
Authors
W.G. Zong, Y.H. Tang, C. Fang, A.A. Xu,