It also provides additional evidence that the nature of the activation and nucleation processes of new particle formation in the clouds of Venus play a very significant role in the ultimate distribution of the clouds.
The two models of fBms (FBM model and FBMINC model) were explored and the differences of the two models are compared from the three aspects: the standard deviation of each step, the small memory and the effect of the number of particles in the cloud.
However, it is essential that the dust dispersion system be designed carefully to ensure that the degree of agglomeration of the particles in the cloud and the cloud turbulence corresponds with the state actually wanted.
However, since the likelihood and process of heterogeneous nucleation depend strongly on the presence and composition of involatile particles in the cloud domain, these difficulties show that an improved characterization and understanding of the CCN are necessary for a complete understanding of the Venus cloud system.
It is shown that the disperse composition and the nonuniform distribution of particles in the cloud are important parameters affecting the detonation propagation mode.
The key factors include the primary particle size distribution of the dust, the degree of de-agglomeration of the dust particles in the cloud, the dust concentration distribution in the cloud, and the cloud turbulence.
But under rain condition, the microwave radiation at 85 GHz is much more sensitive to the raindrops and ice particles in the clouds, and the TB of 85 GHz will descend seriously and become lower than the TB at 37-GHz channel.
The on-board instruments measured everything from temperature to pressure to the size and density of dust and ice particles in the clouds, the researchers gathering streams of information which will later be fed into computer weather models.
Instruments measured the spectrum of water and ice particles in the clouds, air pressure, temperature and electric fields.
