Solar Wind Driven Kinetic Instability In The

Abstract

Solar Wind driven Kinetic Instability in the Earth’s Magnetosphere by using non-Maxwellian kappa and (r, q) Distribution In this thesis, we have comparatively studied of fundamental mode by Using Boltzmann-Vlasov Kinetic model, a current less kinetic instability such as ion acoustic and dust-acoustic using non-Maxwellian distribution. The growth rate and the real frequency are calculated by using kappa (k) and generalized (r, q) distribution and result are compared with those of Maxwellian distribution. In an electrons-ions plasma following a non-Maxwellian generalized distribution function kappa (k) and (r, q), as shown a kinetic instability of ion-acoustic mode exist. In a three species (electrons, ions, dust) plasma following a non-Maxwellian generalized kappa (k) and (r, q) distribution function, as shown that a kinetic instability of dust-acoustic mode exists.