| Mailles 10 | Observation(s) | % des observations totales |
|---|
| E047N667 |
3 | 0.6 |
| E047N669 |
1 | 0.2 |
| E048N667 |
17 | 3.6 |
| E048N668 |
10 | 2.1 |
| E048N669 |
19 | 4 |
| E048N670 |
7 | 1.5 |
| E049N665 |
1 | 0.2 |
| E049N666 |
8 | 1.7 |
| E049N667 |
14 | 3 |
| E049N668 |
3 | 0.6 |
| E049N669 |
5 | 1.1 |
| E049N670 |
1 | 0.2 |
| E049N671 |
16 | 3.4 |
| E049N672 |
2 | 0.4 |
| E050N665 |
3 | 0.6 |
| E050N666 |
4 | 0.8 |
| E050N667 |
6 | 1.3 |
| E050N668 |
5 | 1.1 |
| E050N669 |
5 | 1.1 |
| E050N670 |
2 | 0.4 |
| E050N671 |
2 | 0.4 |
| E050N672 |
1 | 0.2 |
| E051N665 |
1 | 0.2 |
| E051N666 |
9 | 1.9 |
| E051N667 |
5 | 1.1 |
| E051N668 |
11 | 2.3 |
| E051N669 |
14 | 3 |
| E051N670 |
10 | 2.1 |
| E051N671 |
9 | 1.9 |
| E051N672 |
8 | 1.7 |
| E052N664 |
1 | 0.2 |
| E052N665 |
1 | 0.2 |
| E052N666 |
5 | 1.1 |
| E052N667 |
2 | 0.4 |
| E052N668 |
5 | 1.1 |
| E052N669 |
57 | 12.1 |
| E052N670 |
20 | 4.2 |
| E052N671 |
4 | 0.8 |
| E052N672 |
3 | 0.6 |
| E052N673 |
1 | 0.2 |
| E053N663 |
2 | 0.4 |
| E053N664 |
14 | 3 |
| E053N666 |
2 | 0.4 |
| E053N667 |
8 | 1.7 |
| E053N668 |
6 | 1.3 |
| E053N669 |
21 | 4.4 |
| E053N670 |
17 | 3.6 |
| E053N671 |
6 | 1.3 |
| E053N672 |
1 | 0.2 |
| E053N673 |
1 | 0.2 |
| E054N662 |
2 | 0.4 |
| E054N663 |
9 | 1.9 |
| E054N664 |
8 | 1.7 |
| E054N665 |
2 | 0.4 |
| E054N666 |
8 | 1.7 |
| E054N667 |
8 | 1.7 |
| E054N668 |
12 | 2.5 |
| E054N669 |
5 | 1.1 |
| E054N670 |
55 | 11.7 |
| E054N671 |
17 | 3.6 |
| E054N672 |
4 | 0.8 |
| E055N666 |
3 | 0.6 |
| E055N667 |
8 | 1.7 |
| E055N668 |
14 | 3 |
| E055N669 |
1 | 0.2 |
| E055N670 |
18 | 3.8 |
| E056N667 |
5 | 1.1 |
| E056N668 |
2 | 0.4 |
| E057N666 |
1 | 0.2 |