We study particle clustering in a temperature stratified turbulence with
small finite correlation time. It is shown that the temperature stratified
turbulence strongly increases the degree of compressibility of particle
velocity field. This results in the strong decrease of the threshold for the
excitation of the tangling clustering instability even for small particles. The
tangling clustering instability in the temperature stratified turbulence is
essentially different from the inertial clustering instability that occurs in
non-stratified isotropic and homogeneous turbulence. While the inertial
clustering instability is caused by the centrifugal effect of the turbulent
eddies, the mechanism of the tangling clustering instability is related to the
temperature fluctuations generated by the tangling of the mean temperature
gradient by the velocity fluctuations. Temperature fluctuations produce
pressure fluctuations and cause particle clustering in regions with increased
pressure fluctuations. It is shown that the growth rate of the tangling
clustering instability is much larger than that of the inertial clustering
instability. It is found that depending on the parameters of the turbulence and
the mean temperature gradient there is a preferential particle size at which
the particle clustering due to the tangling clustering instability is more
effective. The particle number density inside the cluster after the saturation
of this instability can be in several orders of magnitude larger than the mean
particle number density. It is also demonstrated that the evaporation of
droplets drastically change the tangling clustering instability, e.g., it
increases the instability threshold in the droplet radius. The tangling
clustering instability is of a great importance, e.g., in atmospheric
turbulence with temperature inversions.Comment: 13 pages, 7 figures, REVTEX4-1, revised versio