| Mailles 10 | Observation(s) | % des observations totales |
|---|
| E047N667 |
1 | 0.8 |
| E048N667 |
12 | 9.8 |
| E048N668 |
7 | 5.7 |
| E048N669 |
14 | 11.4 |
| E048N670 |
1 | 0.8 |
| E049N665 |
6 | 4.9 |
| E049N666 |
6 | 4.9 |
| E049N667 |
9 | 7.3 |
| E049N668 |
1 | 0.8 |
| E049N671 |
2 | 1.6 |
| E050N665 |
11 | 8.9 |
| E050N666 |
3 | 2.4 |
| E050N667 |
2 | 1.6 |
| E050N668 |
3 | 2.4 |
| E050N669 |
5 | 4.1 |
| E051N665 |
1 | 0.8 |
| E051N668 |
3 | 2.4 |
| E051N669 |
1 | 0.8 |
| E052N668 |
1 | 0.8 |
| E052N670 |
4 | 3.3 |
| E052N671 |
1 | 0.8 |
| E053N665 |
1 | 0.8 |
| E053N666 |
2 | 1.6 |
| E053N667 |
1 | 0.8 |
| E053N669 |
3 | 2.4 |
| E053N670 |
2 | 1.6 |
| E054N669 |
2 | 1.6 |
| E054N670 |
22 | 17.9 |
| E054N671 |
4 | 3.3 |
| E055N667 |
1 | 0.8 |
| E055N668 |
2 | 1.6 |
| E055N670 |
4 | 3.3 |
|
2 | 1.6 |