Velocity Structure of Bright Points in a Coronal Hole

Details Velocity Structure of Bright Points in a Coronal Hole Velocity Structure of Bright Points in a Coronal Hole

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..397...35k&link_type=abstract

First Results From Hinode ASP Conference Series, Vol. 397, Proceedings of the conference held 20-24 August, 2007, at Trinity Col

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the velocity structure of bright points in the corona and in the transition region. This is one of the first results from the coordinated observation with Hinode/EIS and SOHO/SUMER in April 2007. Bright points in the corona are associated with bright patches in the transition region network. The result suggests coronal bright points are rooted in the magnetic field concentration of the network. No clear connection is found between velocities in the corona and the transition region, but observing time difference between EIS and SUMER could be the cause of the dissociation.

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