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Abstract: The activity and structure of daytime summer streams of the Taurid meteor complex, Zeta Perseids and Beta Taurids, based on radio observations carried out by Bologna-Lecce-Modra forward scatter system and Ondřejov backscatter meteor radar in 1997-2005 are analysed and discussed. The observations indicate a filamentary structure of the streams supported also by the mass exponent values derived for individual returns.
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Last update: February 06, 2007