Effects of Grain Size on the Bremsstrahlung Spectrum of Electron-Dust Grain Collisions in Dusty Plasmas

The hardness values extracted by employing the volume fraction model (Fig. 9a) and the relative change in hardness (Fig. 9b) are in line with general behavior discussed

In a first step, slabs of different steel grades were investigated to determine the prior austenite grain size, followed by a feasibility study on the simulation of austenite

Similar to the sediment record from the Paci fi c sector of the Southern Ocean, increased Fe and terrestrial biomarker accumu- lation during glacial periods indicates enhanced

The influence of deformation temperature on the microstructural evolution of an austenitic stainless steel with an initial grain size of 120 μm, deformed to =57% with a strain-rate of ˙

Distribution of balloelectric ions according to the number of water molecules A, B, C ja D are levels of neutralizing ionization in the laboratory experiment.. Distribution

Advanced methods like the Warren-Averbach analysis [2] allow the determination of a volume and an area averaged mean grain size and so enable to calculate the width of the

The results show that as the grain size increases, both the impedance and the permittivity of the films decrease, whereas the conductivity shows an inverse variation.. The Z ∗ plane

Hence, we have found that the grain size effect plays a significant role in the electron-dust grain bremsstrahlung process in dusty plasmas containing highly charged dusty