Image Details
Caption: Fig. 6.
Artificial IO VI λ1037 latitudinal profiles, synthesized from our models 1 (left) and 2 (right), assuming different oxygen abundances in the streamer closed region (core) relative to photospheric values. The profiles are taken along a line perpendicular to the streamer axis, at the height of the center of the streamer core, 1.75 ﹩R_{\odot }﹩ (left) and 2.0 ﹩R_{\odot }﹩ (right).
© 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.