Table 3
Power-law exponents of the distribution n(m)·m·a.
Regime | δ i | |
ai < asett | ai ≥ asett | |
|
||
Brownian motion regime |
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Turbulent regime I |
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0 |
Turbulent regime II |
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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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