CAOSP abstracts, Volume: 22, year: 1992
- Author(s): RUSIN, V.; KLOCOK, L.; ZIMMERMANN, P.; RYBANSKY, M.; SYKORA, J.;
MINAROVJECH, M.
- Journal: Contributions of the Astronomical Observatory Skalnate Pleso,
vol. 22, p. 117-122.
- Date: 07/1992
- Title: Summary report of the Astronomical Institute Observations during the
July 11, 1991 eclipse
- Keyword(s): SUN, CORONA, ECLIPSES
- Pages: 117 -- 122
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.
Full text version of this article in
PDF.
