In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 1
D. Pecinová - P. Pecina
Detaily:
Rok, strany: 2008, 12 - 20
Kľúčové slová:
physics of meteors, radar meteors, range distribution, ionization coefficient
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2008/Vol_38/No_1/pp12-20_abstract.html
O článku:
The theoretical radar meteors Range Distribution Model of the overdense
observed range distributions of meteors belonging to the Quadrantid,
Perseid, Leonid, Geminid, γ Draconid (Giacobinid), ζ Perseid
and β Taurid streams to study the dependence of the ionization
coefficient β on the meteoroid atmospheric velocity. The dependence
in question is studied and confronted with the analogous dependence
obtained by other authors. Also the mathematical form of a new dependence
is evaluated and presented.
Ako citovať:
ISO 690:
Pecinová, D., Pecina, P. 2008. Radar meteors range distribution model. IV. Ionization coefficient. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.1, pp. 12-20. 1335-1842.
APA:
Pecinová, D., Pecina, P. (2008). Radar meteors range distribution model. IV. Ionization coefficient. Contributions of the Astronomical Observatory Skalnaté Pleso, 38(1), 12-20. 1335-1842.