Astronomy and Astrophysics – Astronomy
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.9427l&link_type=abstract
American Astronomical Society Meeting 210, #94.27; Bulletin of the American Astronomical Society, Vol. 39, p.221
Astronomy and Astrophysics
Astronomy
Scientific paper
The combination of multi-wavelength, high resolution, high cadence data from the Hinode X-Ray Telescope (XRT) and the Transition Region And Coronal Explorer (TRACE) give an unprecedented view of solar active region dynamics and coronal topology. We focus on examples of filament structures observed by TRACE and XRT in December 2006 and February 2007. Co-alignment of observations in these two instruments yields a striking picture of the coronal structures, with loops lying both along and above the filament. Overlying loops exhibit remarkable dynamics while the filament lies dormant, and numerous x-point and triple-leg structures undergo repeated brightenings. We also employ magnetic field data from SOT and from SOLIS to compare a non-linear force-free model of the coronal magnetic field with the observed loops.
DeLuca Edward E.
Kano Ryouhei
Lundquist Loraine L.
Narukage Noriyuki
Reeves Katharine K.
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