Table J-3: Cumulative number of impacts, N, to a randomly oriented plate for a range of minimum particle sizes using the MASTER-2005 model

Diameter (cm)

Ndeb(m-2yr-1)

Nmet(m-2yr-1)

Ntot(m-2yr-1)

0,0001

3,41E+3

9,97E+2

4,41E+3

0,0002

2,09E+3

6,01E+2

2,69E+3

0,0003

1,81E+3

5,16E+2

2,33E+3

0,0005

1,48E+3

4,44E+2

1,93E+3

0,0007

1,31E+3

3,14E+2

1,63E+3

0,001

9,25E+2

2,03E+2

1,13E+3

0,002

4,22E+2

7,88E+1

5,01E+2

0,003

2,34E+2

3,60E+1

2,70E+2

0,005

1,24E+2

1,13E+1

1,35E+2

0,007

7,67E+1

4,98E+0

8,17E+1

0,01

3,88E+1

2,15E+0

4,10E+1

0,02

4,87E+0

3,61E-1

5,23E+0

0,03

6,10E-1

9,28E-2

7,03E-1

0,05

2,76E-2

1,75E-2

4,50E-2

0,07

4,52E-3

5,24E-3

9,76E-3

0,1

1,51E-3

1,37E-3

2,89E-3

0,2

4,79E-4

1,14E-4

5,93E-4

0,3

2,78E-4

1,82E-5

2,96E-4

0,5

1,06E-4

2,88E-6

1,09E-4

0,7

6,81E-5

7,50E-7

6,89E-5

1,0

3,53E-5

1,60E-7

3,55E-5

2,0

1,11E-5

-

1,15E-5

3,0

7,80E-6

-

7,80E-6

5,0

4,60E-6

-

4,60E-6

10,0

3,19E-6

-

3,19E-6

NOTE:  The results are for an altitude h = 800 km, inclination i = 98°, and the epoch May 1st, 2005. For meteoroids a density of ρ = 2,5 g cm-3 was used to convert masses to diameters.