In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 3
Z. Kaňuchová - J. Svoreň
Detaily:
Rok, strany: 2008, 501 - 518
Kľúčové slová:
Geminids, structure of the meteoroid stream, photographic meteor orbits
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2008/Vol_38/No_3/pp501-518_abstract.html
O článku:
249 out of 387 selected Geminids are formally grouped into one of the 16
determined orbital filaments. A structure of the filaments is studied.
As it was expected, the Geminids seem to be a relatively compact stream.
Only a weak conception of 4 branches of filaments can be found. It is
hardly cognizable only on the basis of the space visualisation and
with the low numerous filaments included. According to our analysis,
the two observed maxima of Geminids (e. g. Ryabova, 2001a)
are product of the activity of two different groups of filaments.
These parts of Geminids might appear to be as two different meteor
streams, unless the similarity of their orbits was so high.
Ako citovať:
ISO 690:
Kaňuchová, Z., Svoreň, J. 2008. Looking for the Geminids structure in the range of photographic meteors. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.3, pp. 501-518. 1335-1842.
APA:
Kaňuchová, Z., Svoreň, J. (2008). Looking for the Geminids structure in the range of photographic meteors. Contributions of the Astronomical Observatory Skalnaté Pleso, 38(3), 501-518. 1335-1842.