Observations Of Filament Channels By Hinode/XRT And STEREO/EUVI

Details Observations Of Filament Channels By Hinode/XRT And STEREO/EUVI Observations Of Filament Channels By Hinode/XRT And STEREO/EUVI

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.1013s&link_type=abstract

American Astronomical Society, SPD meeting #40, #10.13; Bulletin of the American Astronomical Society, Vol. 41, p.825

Astronomy and Astrophysics

Astronomy

Scientific paper

We will present preliminary results of an investigation on filament channels observed by Hinode/XRT and STEREO/EUVI. We selected 8 filament channels that are located in active region remnants. Filament channels 1, 2 and 3 appear to be the same channel observed at different solar rotations, and channels 5, 6, 7 and 8 are also the same channel at different solar rotations. We study the X-ray and EUV structures as well as the evolution of these channels observed by Hinode/XRT and STEREO/EUV. The corresponding H-alpha filament information is provided by KSO and MLSO. In order to understand the magnetic configuration of filament channels, we will also explore non-linear force-free field modeling of two selected filament channels. The modeling is based on flux rope insertion method, and the magnetic field information is provided by SOLIS.

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