All Tables

Table 1: Observing periods in years 2000-2002. Time periods of each year are labeled with the beginning day in Nov., bd, the end day, ed, the beginning hour and minute, bh and bm, and end hour and minute, eh and em, respectively of each particular period, in UT, and with the corresponding solar longitudes, $bL_{\odot }$ and $eL_{\odot }$ [J2000.0]. The last column indicates whether the period was considered a background (i.e. b) or shower (i.e. s) activity. These periods were the same for all 4 categories of echoes except for 2000 when also the interval from $L_{\odot} = 234\hbox{$.\!\!^\circ$ }85$ to $L_{\odot} = 235\hbox{$.\!\!^\circ$ }46$ was used as a background for echoes having $T \! \geq \! 10.0$ s.
Table 2: Positions of main activity peaks recorded in 2000. The instants of the maxima are determined with an error of 15 min. Our observations corresponding to the forecast of Asher & McNaught (2000) are presented in bold (see Sect. 5.1).
Table 3: Positions of main activity peaks recorded in 2001. The instants of the maxima are determined with an error of 15 min. Our observations corresponding to the forecast of Jenniskens (2001) and Lyytinen et al. (2001) are presented in bold (see Sect. 5.2).
Table 4: Positions of main activity peaks recorded in 2002. The instants of the maxima are determined with an error of 15 min. Our observations corresponding to the forecast of Jenniskens (2001), McNaught & Asher (2002) and Vaubaillon (2002) are presented in bold (see Sect. 5.3).
Table 8: Mass of a meteoroid as a function of time and duration, T. Meteoroid mass is in 10^-6 kg.
Table 5: Mass distribution index, s, computed by means of formula (1), valid for 2000. Only indices whose standard deviations do not exceed $10 \%$ percentage of the index itself are shown. The index was computed within 30-min time intervals the midpoints of which are presented in the table. The first column contains the day in Nov, the second and third one contains hour, h, and minute, m, of the corresponding beginning time, in UT. Also solar longitude of the middle of corresponding span, $L_{\odot }$ , is presented. The last but one column contains the values of s while the last one contains standard deviation, s.d. of s.
Table 6: The same as in Table 5 but for 2001.
Table 7: The same as in Table 5 but for 2002.