Turbulent Gravito-Electrostatic Sheath (GES) Structure with Kappa-Distributed Electrons for Solar Plasma Characterization

Athermal GES-based solar plasma stability with sphero-logabarotropic special effects

“…It has further theoretically been demonstrated that the non-thermal non-extensive electronic thermostatistics reduces the bounded GES field strength by 21.67% and the corresponding potential by 30%, and so forth [10]. In addition, it has specifically been shown herewith that the diffused SSB extension gets slightly enhanced radially outward due to the electronic non-thermality factors, and so on [12].…”

“…The thermostatistical non-thermal non-ideality effects here are basically caused by diversified equilibrium gradient forces and zeroth-order inhomogeneity sources in diversified astrospace environments as predicted by various multi-spaced satellite observations [10][11][12]15,16]. It is to note that the long-range gravito-electrostatic force couples the bounded SIP and unbounded SWP via the interfacial coupling SSB.…”

“…important outcome of such rigorous investigations is that the entire GES model structure gets drastically modified due to the non-thermal non-ideality effects caused by diversified equilibrium gradient forces and zeroth-order inhomogeneity sources [10][11][12]. It has further theoretically been demonstrated that the non-thermal non-extensive electronic thermostatistics reduces the bounded GES field strength by 21.67% and the corresponding potential by 30%, and so forth [10].…”

“…Physical model and formalism. -An abridged bi-fluidic quasi-neutral solar plasma system is considered in a spherically symmetric non-thermal GES model fabric [10][11][12]. The exclusion of non-radial polar and azimuthal coordination counterparts helps us avoid mathematical complications in our analysis.…”

“…The exclusion of non-radial polar and azimuthal coordination counterparts helps us avoid mathematical complications in our analysis. It compositionally contains the non-thermal κ-distributed lighter electrons and hydrodynamically treated heavier ions in the limiting case of the asymptotical zero-value of the fluid mean free paths [12]. It is noteworthy that the bulk thermodynamic characteristics of our plasma model system here are attributable to the lighter electronic species only against the heavier ionic species.…”