In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 37, no. 2
D. Pecinová - P. Pecina
Details:
Year, pages: 2007, 83 - 106
About article:
The theoretical construction of a model of the range distribution of
computation of five important parameters connected with the structure
of meteor showers as well as physical features of meteoroids related
to them. These are: the mass distribution index, s, the shower flux
density, Θm0, the ionization coefficient,
β, the Levin's
parameter (self-similarity parameter), µ, the product of the
shape-density coefficient, K, and the ablation parameter, σ.
We present details of the numerical model in the article which proved
to be a good explanation for the real observed process. The model (RaDiM)
is based on the overdense echoes of shower meteors. It makes use of the
long-term series of data that have been collected by the Ondřejov
meteor radar during almost five decades. Its application and relevant
results will be described in subsequent articles.
How to cite:
ISO 690:
Pecinová, D., Pecina, P. 2007. Radar meteors range distribution model. I. Theory. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 37, no.2, pp. 83-106. 1335-1842.
APA:
Pecinová, D., Pecina, P. (2007). Radar meteors range distribution model. I. Theory. Contributions of the Astronomical Observatory Skalnaté Pleso, 37(2), 83-106. 1335-1842.