Progress in the study of dusty plasmas

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Dusty plasma effects in Saturn's magnetosphere (2004, background): “…(that by themselves can be further complicated if a grain is embedded in a multispecies plasma with non-Maxwellian energy distributions), grains can charge because of a number of other processes, including photoelectron and secondary and thermionic electron emissions [Whipple, 1981; Mendis, 2002].”
Nonlinear waves and structures in dusty plasmas (2002, background): “Dust exists in most space and laboratory plasmas (Goertz 1989, Mendis and Rosenberg 1994, Winter 1998, Bouchoule 1999, Hollenstein 2000, Verheest 2000, Mendis 2002, Shukla and Mamun 2002).”
Complex (dusty) plasmas: current status, open issues, perspectives (2005, background): “These processes are of importance for dust charging in the working body of solid-fuel MHD generators and rocket engines [40,114–116], in the upper atmosphere, in space [4,117,118], and in some laboratory experiments, for instance, in thermal plasmas [16,41–49] or in plasmas induced by UV irradiation”