Table 4.

Space-time power distribution P₁(l, s, t | s*, t*) for the Cluster A (s* = 1) on Day 31 (t* = 1) with high risk (RR= 9. 91), where t is a temporal length of detected cluster. The mark "*" is the powers of accurate detection.

(A) flexible (K = 20)
	includes s assumed areas
	0			1
	29-	30-	31-	29-	30-	31-
length l of areas	t = 3	2	1	t = 3	2	1	total
1	0	0	0	0	6	*315	321
2	0	0	0	0	1	50	51
3	0	0	0	1	2	34	37
4	0	0	0	1	6	34	41
5	0	0	0	2	5	48	55
6	1	0	0	2	2	51	56
7	1	0	0	4	13	35	53
8	0	1	0	1	12	28	42
9	1	1	2	5	6	28	43
10	0	0	0	2	7	22	31
11	1	0	0	1	4	8	14
12	1	1	2	1	0	10	15
13	0	0	0	1	1	2	4
14	0	0	0	0	0	1	1
15	0	0	0	0	0	0	0
16	0	0	0	0	0	0	0
17	0	0	0	0	0	0	0
18	0	0	0	0	0	0	0
19	0	0	0	0	0	0	0
20	0	0	0	0	0	0	0
total	5	3	4	21	65	666	764
(B) cylindrical (K = 20)
	includes s assumed areas
length l of areas	0			1
	29-	30-	31-	29-	30-	31-
	t = 3	2	1	t = 3	2	1	total
1	0	0	0	5	18	*697	720
2	0	0	0	5	4	63	72
3	0	0	0	1	2	18	21
4	0	0	0	0	4	10	14
5	0	0	0	0	0	2	2
6	1	0	0	1	0	3	5
7	1	0	0	1	1	1	4
8	2	0	0	0	1	1	4
9	0	1	1	0	0	2	4
10	0	0	0	0	0	0	0
11	0	0	0	0	0	1	1
12	0	0	0	0	0	0	0
13	0	0	0	0	0	0	0
14	0	0	0	0	0	2	2
15	0	0	0	0	1	3	4
16	0	0	0	0	0	0	0
17	0	0	0	2	0	1	3
18	1	0	0	0	0	1	2
19	0	0	0	0	0	1	1
20	0	0	0	0	0	1	1
total	5	1	1	15	31	807	860