“…It is noticed that VCDF is reducible to Maxwellian distribution function when simultaneously α = 0 and κ ⟶ ∞ [6,17,18]. The dispersion and damping/growth characteristics of numerous plasma waves and instabilities have been studied from the utilization of Vasyliunas-Cairns distribution in several natural environments such as plasma sheets and heliospheric (inner and outer heliospheric, solar wind) regimes [6,17,18,[36][37][38][39][40][41][42][43][44] . It has been observed that these non-thermal distributions for the population of non-thermal particles could include temperature anisotropy, i.e., contrasting perpendicular and parallel temperatures (T ⊥p ≠ T ∥p ) due the naturally occurring phenomena of compression and rarefaction in the large extended space plasmas [5,11,13,14,16,26,30].…”