Dust Successive Generations in Ar/SiH4: Dust Cloud Dynamics

We use a vortex shaker to test respirable dust generation from eight powders with similar physical properties except their particle size distributions which differ from each

[ 59 ] In the particular case of the OMEGA storm, LMD- MMM simulations demonstrate that local dust storms have the ability to form detached layer of dust through radiatively

Here, we present the results from an additional simulated data set in order to shed light on the capacity of the moments expansion on β to capture the complexity arising

Histograms of the parameters derived for each dust model (relative dust abundances, intensity of the radiation field, and relative intensity of the NIR continuum, see Sect. 4.2) in

In a previous paper [37], we showed that the formation and growth of dust successive generations in Ar/SiH 4 low pressure plasmas is a cyclic phenomenon, involving three steps,

The delivery instability is directly linked to the growth of a new generation of dust particles inside the void which trigger strong oscillations of its size. We showed that the

From figures 2(c) and 2(d), we conclude that lots of "small" particles (around 10 nm in diameter) are deposited in the discharge center, while the deposition becomes less