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The spreading disks, mostly tiny ice particles, with some ice boulders for heft, had never before been seen in such rich detail.
Very fine spherical CoFe2O4 particles with some extent of aggregation can be observed in the SEM pictures.
TEM showed that TiO2 particles with some agglomerates were dispersed over the surface of fullerene together with WO3 particles.
The samples are all composed of well-dispersed spherical particles with some small particles adhering to their surface.
The methodology for investigation of the interaction between neighbouring particles with some amount of viscoelastic material between them is explained.
The SEM results show that the pure Ni(OH 2 and Co-substituted sample display spherical particles with some degree of agglomeration.
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In fact, a particle with some properties opposite to those of physicists' current favorite dark matter candidate the weakly interacting massive particle, or WIMP would do just as good a job at explaining the stuff, a quartet of theorists says.
Both studies from Kugler and Leta.[ 41] and Psarras et al.[ 22] observed a uniform distribution of V throughout an individual catalyst particle with some indication of preferential residence in zeolite domains.
Inhomogeneous, spherical particles along with some chunky particles were observed for ZnOW.
Scanning electron microscopy images show that Co3O4 thin film is composed of spherical-like coarse particles, together with some pores among particles.
Although there was some melting occurred at the particles surface with some solute segregation found in the vicinity close to the surface, intermetallic compounds were not observed.
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