Deposition, in physics, is a process where aerosol particles collect or deposit onto solid surfaces. It can be divided into two sub-processes: dry and wet deposition. Deposition decreases the concentration of aerosol particles in the air. The rate of deposition, or the deposition velocity is slowest for particles of intermediate size, because mechanisms for deposition are most effective for either small or large particles.
Deposition velocity is defined as: F = v*c, where F is flux density, v is deposition velocity and c is concentration.
In gravitational deposition this velocity is settling velocity due to the gravity and drag.
It is often studied whether or not the particle will impact an obstacle. This can be predicted with the Stokes number: Stk = S/d, where S is stopping distance, which depends on particle size, velocity, and drag forces; d is characteristic size, often the diameter of the obstacle. If Stk is smaller than 1 the particle will not collide with that obstacle, and if it is much larger than 1 it will.
Deposition due to Brownian motion obeys Ficks first and second law, and the resulting depostion flux is: J=n*(D/πt)¹/², where J is deposition flux, n is concentration at the beginning, D is diffusion constant and t is time. This can be integrated to determine the concentration at each moment of time.
Dry deposition is caused by:
In wet deposition, there are always some atmospheric hydrometeors which scavenge aerosol particles. This means that dry deposition is gravitational coagulation with water droplets. Different types of wet deposition include:
see also Condensation in aerosol dynamics
This article is licensed under the GNU Free Documentation License.
It uses material from the
"Deposition (Aerosol physics)".
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