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.
Contributions of the Astronomical Observatory Skalnate Pleso
- Pub Date:
- July 1992