In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 39, no. 1
P. Zigo - V. Porubčan - G. Cevolani - G. Pupillo
Detaily:
Rok, strany: 2009, 5 - 17
Kľúčové slová:
meteor showers, radio observations
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2009/Vol_39/No_1/pp5-17_abstract.html
O článku:
The activity and mass distribution of the Geminid meteor shower of 1996 -
2007 based on radio observations by a forward-scatter system operating along
the Bologna - Modra baseline are analysed and presented. Activity curves
corrected for an observability function derived for the system indicate a
multiple-peak structure of the shower.The global activity curve for
overdense echoes of durations ≥1s and ≥8s depicts two
peaks at solar longitude 261.7°, 262.3° and 261.9°, 262.3°,
respectively. Larger particles are concentrated more to the centre of the
shower and slightly shifted towards the descending branch of the shower
activity. The mean mass exponent of the Geminids is 1.73.
Ako citovať:
ISO 690:
Zigo, P., Porubčan, V., Cevolani, G., Pupillo, G. 2009. The activity and mass distribution of the Geminid meteor shower of 1996-2007 from forward scatter radio observations. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 39, no.1, pp. 5-17. 1335-1842.
APA:
Zigo, P., Porubčan, V., Cevolani, G., Pupillo, G. (2009). The activity and mass distribution of the Geminid meteor shower of 1996-2007 from forward scatter radio observations. Contributions of the Astronomical Observatory Skalnaté Pleso, 39(1), 5-17. 1335-1842.