Outflow Velocities at the Base of a Polar Coronal Hole During the 1998 Total Eclipse

Details Outflow Velocities at the Base of a Polar Coronal Hole During the 1998 Total Eclipse Outflow Velocities at the Base of a Polar Coronal Hole During the 1998 Total Eclipse

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ssrv...87..291p&link_type=abstract

Space Science Reviews, v. 87, Issue 1/2, p. 291-294 (1999).

Physics

1

Sun, Corona, Coronal Holes, Flows

Scientific paper

Polar coronal holes represent the most convincing site from which the high-speed solar wind originates. Here we report high-accuracy Doppler shifts measured in the O VI (1037.6 Å) line obtained by SUMER on SOHO inside an interplume region within the south polar coronal hole. We infer limits on the outflow velocity and draw hints about the flow geometry.

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