The Double Structure of the Coronal Streamer Belt

Details The Double Structure of the Coronal Streamer Belt The Double Structure of the Coronal Streamer Belt

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006soph..235..331e&link_type=abstract

Solar Physics, Volume 235, Issue 1-2, pp. 331-344

Physics

3

Scientific paper

Increasing the effective spatial resolution when analyzing LASCO-C2/SOHO data helped to reveal the existence of double-ray structure in the streamer belt, both in the absence and presence of belt bends. Streamer-belt rays located in the plane of the sky are demonstrated to deviate poleward (north- and southward, respectively, in the N and S hemispheres) at distances R < 4{ }5R &sun; from the Sun center. These new results concerning streamer belt structure are important as the basis for checking a theory claiming to adequately describe physical processes in the corona.

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