Mailles 10 | Observation(s) | % des observations totales |
E048N667 |
16 | 3.2 |
E048N668 |
22 | 4.4 |
E048N669 |
7 | 1.4 |
E048N670 |
17 | 3.4 |
E049N665 |
2 | 0.4 |
E049N667 |
15 | 3 |
E049N668 |
7 | 1.4 |
E049N669 |
1 | 0.2 |
E049N670 |
20 | 4 |
E049N671 |
4 | 0.8 |
E050N665 |
1 | 0.2 |
E050N667 |
9 | 1.8 |
E050N668 |
28 | 5.7 |
E050N669 |
7 | 1.4 |
E050N670 |
6 | 1.2 |
E050N671 |
5 | 1 |
E050N672 |
4 | 0.8 |
E051N667 |
1 | 0.2 |
E051N668 |
6 | 1.2 |
E051N669 |
4 | 0.8 |
E051N670 |
1 | 0.2 |
E051N671 |
12 | 2.4 |
E051N672 |
23 | 4.6 |
E051N673 |
2 | 0.4 |
E052N666 |
10 | 2 |
E052N667 |
9 | 1.8 |
E052N668 |
30 | 6.1 |
E052N669 |
6 | 1.2 |
E052N670 |
4 | 0.8 |
E052N671 |
7 | 1.4 |
E052N672 |
8 | 1.6 |
E052N673 |
4 | 0.8 |
E053N664 |
1 | 0.2 |
E053N667 |
31 | 6.3 |
E053N668 |
18 | 3.6 |
E053N669 |
2 | 0.4 |
E053N670 |
10 | 2 |
E053N671 |
14 | 2.8 |
E053N672 |
12 | 2.4 |
E053N673 |
3 | 0.6 |
E054N663 |
1 | 0.2 |
E054N664 |
4 | 0.8 |
E054N666 |
11 | 2.2 |
E054N667 |
8 | 1.6 |
E054N668 |
2 | 0.4 |
E054N670 |
58 | 11.7 |
E054N671 |
24 | 4.8 |
E054N672 |
6 | 1.2 |
E055N666 |
10 | 2 |
E055N667 |
1 | 0.2 |
E055N668 |
4 | 0.8 |
E055N670 |
10 | 2 |
E056N666 |
2 | 0.4 |
E056N667 |
7 | 1.4 |
E057N667 |
4 | 0.8 |
|
1 | 0.2 |