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Formation Heights of Extreme Ultraviolet Lines in an Active Region Derived by Correlation of Doppler Velocity and Magnetic Field View all abstracts by submitter

Yang Guo   Submitted: 2010-03-11 03:52

We study the correlation heights, which indicate the formation heights of Extreme Ultraviolet (EUV) lines in an active region using observations from the EUV Imaging Spectrometer (EIS) and Solar Optical Telescope (SOT) on board Hinode. The nonlinear force-free field (NLFFF) optimization method is adopted to extrapolate the 3D magnetic fields to higher layers. Three subregions with different characteristics are selected in the active region for this study. The results show that the formation heights in different subregions vary with their different magnetic fields or velocity patterns. After solving the line blending problem between the He 2 256.32 Å and Si 10 256.37 Å lines by the double Gaussian curve fitting, we find that the transition region lies higher in a strong magnetic area. In a pre-flare heating area there possibly exist multithermal loops as implied by comparing the Doppler velocity and the magnetic field on the solar disk.

Authors: Guo, Y., Ding, M. D., Jin, M., Wiegelmann, T.
Projects: Hinode/EIS,Hinode/SOT

Publication Status: ApJ (2009), 696, 1526
Last Modified: 2010-03-12 09:44
Go to main E-Print page  Soft X-ray coronal spectra at low activity levels observed by RESIK  Magnetic Field Structures in a Facular Region Observed by THEMIS and Hinode   Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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