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.
2000
day h m $L_{\odot }$ s s.d.
17 $\hspace{1.6mm}1$ 15 $234\hbox{$.\!\!^\circ$ }98$ 1.60 0.14
17 $\hspace{1.6mm}1$ 45 $235\hbox{$.\!\!^\circ$ }00$ 1.76 0.17
17 $\hspace{1.6mm}2$ 45 $235\hbox{$.\!\!^\circ$ }04$ 1.71 0.16
17 $\hspace{1.6mm}3$ 45 $235\hbox{$.\!\!^\circ$ }08$ 1.62 0.13
17 $\hspace{1.6mm}6$ 15 $235\hbox{$.\!\!^\circ$ }19$ 1.88 0.07
17 $\hspace{1.6mm}6$ 45 $235\hbox{$.\!\!^\circ$ }21$ 1.02 0.05
17 $\hspace{1.6mm}7$ 45 $235\hbox{$.\!\!^\circ$ }25$ 2.19 0.13
17 $\hspace{1.6mm}8$ 15 $235\hbox{$.\!\!^\circ$ }27$ 2.36 0.15
17 $\hspace{1.6mm}8$ 45 $235\hbox{$.\!\!^\circ$ }29$ 2.54 0.17
17 $\hspace{1.6mm}9$ 15 $235\hbox{$.\!\!^\circ$ }32$ 3.65 0.29
17 11 45 $235\hbox{$.\!\!^\circ$ }42$ 2.18 0.19
17 13 45 $235\hbox{$.\!\!^\circ$ }88$ 1.61 0.10
18 $\hspace{1.6mm}0$ 45 $235\hbox{$.\!\!^\circ$ }97$ 1.48 0.14
18 $\hspace{1.6mm}1$ 15 $235\hbox{$.\!\!^\circ$ }99$ 1.51 0.09
18 $\hspace{1.6mm}1$ 45 $236\hbox{$.\!\!^\circ$ }01$ 1.40 0.03
18 $\hspace{1.6mm}2$ 15 $236\hbox{$.\!\!^\circ$ }03$ 1.21 0.05
18 $\hspace{1.6mm}2$ 45 $236\hbox{$.\!\!^\circ$ }05$ 1.16 0.05
18 $\hspace{1.6mm}3$ 15 $236\hbox{$.\!\!^\circ$ }07$ 1.14 0.02
18 $\hspace{1.6mm}3$ 45 $236\hbox{$.\!\!^\circ$ }09$ 1.13 0.03
18 $\hspace{1.6mm}4$ 15 $236\hbox{$.\!\!^\circ$ }11$ 1.20 0.06
18 $\hspace{1.6mm}4$ 45 $236\hbox{$.\!\!^\circ$ }13$ 1.16 0.03
18 $\hspace{1.6mm}5$ 15 $236\hbox{$.\!\!^\circ$ }16$ 1.21 0.05
18 $\hspace{1.6mm}5$ 45 $236\hbox{$.\!\!^\circ$ }18$ 1.22 0.05
18 $\hspace{1.6mm}6$ 15 $236\hbox{$.\!\!^\circ$ }20$ 1.27 0.02
18 $\hspace{1.6mm}6$ 45 $236\hbox{$.\!\!^\circ$ }22$ 1.28 0.01
18 $\hspace{1.6mm}7$ 15 $236\hbox{$.\!\!^\circ$ }24$ 1.51 0.02
18 $\hspace{1.6mm}7$ 45 $236\hbox{$.\!\!^\circ$ }26$ 1.57 0.03
18 $\hspace{1.6mm}8$ 15 $236\hbox{$.\!\!^\circ$ }28$ 1.54 0.03
18 $\hspace{1.6mm}8$ 45 $236\hbox{$.\!\!^\circ$ }30$ 2.12 0.14
18 $\hspace{1.6mm}9$ 15 $236\hbox{$.\!\!^\circ$ }32$ 1.34 0.12
18 $\hspace{1.6mm}9$ 45 $236\hbox{$.\!\!^\circ$ }34$ 1.39 0.11
18 10 15 $236\hbox{$.\!\!^\circ$ }37$ 1.77 0.18


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