Fine Structure of a Coronal Bright Point as Seen with SoHO, TRACE, and Hinode

Details Fine Structure of a Coronal Bright Point as Seen with SoHO, TRACE, and Hinode Fine Structure of a Coronal Bright Point as Seen with SoHO, TRACE, and Hinode

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..415..140p&link_type=abstract

The Second Hinode Science Meeting: Beyond Discovery-Toward Understanding ASP Conference Series, Vol. 415, proceedings of a meeti

Astronomy and Astrophysics

Astronomy

Scientific paper

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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