CAOSP abstracts, Volume: 22, year: 1992

Abstract: A brief description of the scientific goals and preliminary results related to the 11 July 1991 eclipse at La Paz is given. The white-light corona was a maximum type with a very faint, but more complicated structure in the inner corona. Large, well developed helmet streamers were observed in the SW- and NE quadrants extended nearly up to 10 solar radii. No remarkable CME was observed. A plasmoid was seen above the north solar pole.

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