In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 40, no. 3
J. Rybák - R. Mačura - P. Gömöry - A. Kučera
Detaily:
Rok, strany: 2010, 210 - 216
Kľúčové slová:
Sun, astroclimate, Lomnický Peak Observatory
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2010/Vol_40/No_3/pp210-216_abstract.html
O článku:
This contribution presents statistical results on
observations of the solar corona and solar prominences using
coronagraphs at the Lomnický Peak Observatory of the Astronomical
Institute of the Slovak Academy of Sciences in the epoch 1963 -- 2009.
The mean frequency of the observing days in this epoch was 34,93% while
the maximum long-term mean frequency of the observing days was found to be in
the period from August to October.
The mean frequency of the observing days suitable for observations of
prominences was 34,0%, that of the observing days suitable
for observations of the emission corona was 20,03%.
The mean frequency of the observing days in which weather conditions
allowed observations of the emission corona longer than 2 hours
was 13,69%.
Ako citovať:
ISO 690:
Rybák, J., Mačura, R., Gömöry, P., Kučera, A. 2010. Lomnický Peak Observatory - weather and astroclimate. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 40, no.3, pp. 210-216. 1335-1842.
APA:
Rybák, J., Mačura, R., Gömöry, P., Kučera, A. (2010). Lomnický Peak Observatory - weather and astroclimate. Contributions of the Astronomical Observatory Skalnaté Pleso, 40(3), 210-216. 1335-1842.