The reddish rectangular image shows a mid-latitude coronal streamer
observed in the emission of five times ionized oxygen (O VI 103.2 nm)
with UVCS/SOHO.  The green image of the solar disk is made in
Fe XII 19.5 nm emission with EIT/SOHO.  An active region with bright
emission on the limb is located at the base of the streamer observed
at higher heights with UVCS. Both images were made from data obtained
on 22 June 1998 during the rising phase of solar cycle 23.

UVCS observations show that mid-latitude streamers have different
physical properties than the equatorial streamers observed at
solar minimum.  They appear to lack the central O^(5+) depletion
found in equatorial streamers by Raymond et al. (1997, Solar Phys.,
175, 645) and the line of sight 1/e velocities are considerably
smaller than those found in equatorial streamers at solar minimum
by Frazin et al. (1999, Space Sci. Rev., 87, 189).