Accelerated magnetosonic lump wave solutions by orbiting charged space debris

The excitations of nonlinear magnetosonic lump waves induced by orbiting charged space debris particles in the Low Earth Orbital (LEO) plasma region are investigated presence ambient magnetic field. These found to be governed forced Kadomtsev–Petviashvili-type model equation, where forcing term signifies source current generated different possible motions LEO region. Different analytic wave solutions that stable for both slow and fast objects first time. dynamics exact pinned accelerated is explored detail. Approximate with time-dependent amplitudes velocities analysed through perturbation methods types localized functions, yielding approximate solutions. new results may pave directions this field research.