Abstract
Abstract The dissipative propagation due to the dust viscosity of dust nonlinear shock acoustic wave in a collisionless, unmagnetised, oppositely charged viscous dusty plasma with trapped ion has been examined using parameters related to mesosphere and magnetosphere of Jupiter. The modified dissipative Korteweg de Vries–Burgers equation describes the model and solves according to different physical dissipation conditions. The physical effects of two dusty kinematic viscosity coefficients and positively charged dust grains on the shock properties are investigated.
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