Mailles 10 | Observation(s) | % des observations totales |
E048N667 |
1 | 1.9 |
E048N668 |
1 | 1.9 |
E048N669 |
1 | 1.9 |
E049N667 |
2 | 3.8 |
E049N668 |
2 | 3.8 |
E049N670 |
13 | 25 |
E049N671 |
5 | 9.6 |
E050N667 |
1 | 1.9 |
E050N669 |
1 | 1.9 |
E050N671 |
1 | 1.9 |
E051N666 |
1 | 1.9 |
E051N668 |
1 | 1.9 |
E051N669 |
2 | 3.8 |
E051N670 |
1 | 1.9 |
E051N671 |
3 | 5.8 |
E052N666 |
2 | 3.8 |
E052N668 |
1 | 1.9 |
E052N669 |
34 | 65.4 |
E052N670 |
12 | 23.1 |
E052N671 |
3 | 5.8 |
E052N672 |
2 | 3.8 |
E052N673 |
1 | 1.9 |
E053N665 |
1 | 1.9 |
E053N667 |
4 | 7.7 |
E053N668 |
2 | 3.8 |
E053N669 |
4 | 7.7 |
E053N670 |
3 | 5.8 |
E053N671 |
4 | 7.7 |
E054N663 |
2 | 3.8 |
E054N665 |
1 | 1.9 |
E054N668 |
3 | 5.8 |
E054N669 |
2 | 3.8 |
E054N670 |
3 | 5.8 |
E055N666 |
1 | 1.9 |
E055N667 |
2 | 3.8 |
E055N668 |
1 | 1.9 |
E055N669 |
2 | 3.8 |
E055N670 |
2 | 3.8 |