Properties of Coronal Hole/Streamer Boundaries and Adjacent Regions as Observed by SPARTAN 201

Details Properties of Coronal Hole/Streamer Boundaries and Adjacent Regions as Observed by SPARTAN 201 Properties of Coronal Hole/Streamer Boundaries and Adjacent Regions as Observed by SPARTAN 201

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ssrv...87..277m&link_type=abstract

Space Science Reviews, v. 87, Issue 1/2, p. 277-281 (1999).

Physics

4

Scientific paper

The Spartan 201 flights from 1993 to 1995 provided us with observations in H I Lyman-α of several coronal hole/streamer boundaries and adjacent streamers during the declining phase of the current solar cycle: Analysis of the latitudinal dependence of the line intensities clearly shows that there is a boundary region at the coronal hole/streamer interface where the H I Lyman-α intensity reaches a minimum value. Similar results are also found in UVCS/SOHO observations. We also discuss differences in the coronal hole/streamer boundaries for different types of streamers and their changes over the three year period of Spartan 201 observations.

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