Table 3
Power-law exponents of the distribution n(m)·m·a.
| Regime | δ i | |
| ai < asett | ai ≥ asett | |
|
|
||
| Brownian motion regime |
|
|
| Turbulent regime I |
|
0 |
| Turbulent regime II |
|
|
Notes. The slopes were calculated using the formula for a coagulation/fragmentation equilibrium (Eq. (18)). Within each regime of relative velocities, it has to be differentiated whether grains are influenced by settling or not.
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