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Oxygen Abundance in Coronal Streamers

  • Authors: Alberto M. Vásquez and John C. Raymond

Vásquez & Raymond 2005 The Astrophysical Journal 619 1132.

  • Provider: AAS Journals

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).

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