In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 37, no. 2
D. Pecinová - P. Pecina
Detaily:
Rok, strany: 2007, 107 - 124
O článku:
The theoretical radar meteors Range Distribution Model of overdense
to observed range distributions of meteors belonging to the Quadrantid,
Perseid, Leonid, Geminid, γ Draconid (Giacobinid),
ζ Perseid
and β Taurid streams to study the variability of the flux density,
Θm0, and the mass distribution index, s, i.e., the parameters
inherent to the inner structure of meteor streams. With the exception of
the Perseids 1988-1993 no systematic variability of
Θm0 was found in
any of the above-named showers. The values of s were found to be higher
than those of other authors working with radar data and using Kaiser's
formula for its determination. The possible cause is also discussed in
this work. The weighted means of both parameters valid for each stream
were evaluated. They can be considered as representative of each shower.
Ako citovať:
ISO 690:
Pecinová, D., Pecina, P. 2007. Radar meteors range distribution model. II. Shower flux density and mass distribution index. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 37, no.2, pp. 107-124. 1335-1842.
APA:
Pecinová, D., Pecina, P. (2007). Radar meteors range distribution model. II. Shower flux density and mass distribution index. Contributions of the Astronomical Observatory Skalnaté Pleso, 37(2), 107-124. 1335-1842.