UVCS/Spartan Observations of Coronal Streamers

Details UVCS/Spartan Observations of Coronal Streamers UVCS/Spartan Observations of Coronal Streamers

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999eostr..80..263m&link_type=abstract

Eos, Trans., AGU, 80, Spring Mtg. Suppl., S263, 1999

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present H I Lyman alpha observations of coronal streamers obtained by the UVCS instrument aboard Spartan 201 satellite during four flights between 1993 and 1998. The analysis of the data allows us to study the velocity structure of various streamer regions at different phases of the solar activity cycle. We compare physical properties of streamers derived from the UVCS/Spartan H I Lyman alpha measurements before solar minimum with results from UVCS/SOHO and UVCS/Spartan after solar minimum. This work is supported by NASA under Grants NAG 5-613 and 5-3192 to the Smithsonian Astrophysical Observatory.

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