Mailles 10 | Observation(s) | % des observations totales |
E048N667 |
2 | 0.9 |
E048N668 |
4 | 1.9 |
E048N670 |
3 | 1.4 |
E049N667 |
1 | 0.5 |
E049N668 |
4 | 1.9 |
E049N669 |
1 | 0.5 |
E049N670 |
13 | 6.1 |
E049N671 |
12 | 5.7 |
E050N667 |
2 | 0.9 |
E050N668 |
2 | 0.9 |
E050N669 |
5 | 2.4 |
E050N670 |
9 | 4.2 |
E050N671 |
12 | 5.7 |
E051N667 |
8 | 3.8 |
E051N668 |
6 | 2.8 |
E051N669 |
7 | 3.3 |
E051N670 |
7 | 3.3 |
E051N671 |
11 | 5.2 |
E051N672 |
3 | 1.4 |
E052N668 |
2 | 0.9 |
E052N669 |
17 | 8 |
E052N670 |
6 | 2.8 |
E052N671 |
2 | 0.9 |
E052N672 |
1 | 0.5 |
E052N673 |
1 | 0.5 |
E053N664 |
1 | 0.5 |
E053N667 |
7 | 3.3 |
E053N668 |
1 | 0.5 |
E053N669 |
22 | 10.4 |
E053N670 |
1 | 0.5 |
E053N671 |
11 | 5.2 |
E053N672 |
1 | 0.5 |
E054N663 |
1 | 0.5 |
E054N664 |
6 | 2.8 |
E054N667 |
1 | 0.5 |
E054N668 |
3 | 1.4 |
E054N669 |
4 | 1.9 |
E054N670 |
6 | 2.8 |
E054N671 |
1 | 0.5 |
E054N672 |
1 | 0.5 |
E055N667 |
7 | 3.3 |
E055N668 |
3 | 1.4 |
E055N670 |
6 | 2.8 |
E056N666 |
1 | 0.5 |
E056N667 |
1 | 0.5 |
E056N668 |
1 | 0.5 |