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Paper: Fine Structure of a Coronal Bright Point as Seen with SoHO, TRACE, and Hinode
Volume: 415, The Second Hinode Science Meeting: Beyond Discovery-Toward Understanding
Page: 140
Authors: Pérez-Suárez, D.; Maclean, R. C.; Doyle, J. G.; Madjarska, M. S.
Abstract: We present a study of a Coronal Bright Point (BPs) where data from Hinode, SoHO and TRACE are analyzed. Covering a large temperature range, we study the variation of the BP from the surface to the corona investigating both the morphology and variation in physical parameters, such as electron density, Doppler-shift and magnetic field variability. We obtain excellent correlation between the X-ray light curve with the positive magnetic flux; also a good agreement is found between a potential extrapolated magnetic field and the loops seen in the X-ray images.
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