  The excitations of nonlinear magnetosonic waves in presence of charged space
debris in the low Earth orbital plasma region is investigated taking into
account effects of electron inertia in the framework of classical
magnetohydrodynamics, which is also referred to as inertial
magnetohydrodynamics. Magnetosonic waves are found to be governed by a forced
Kadomtsev-Petviashvili equation with the forcing term representing effects of
space debris particles. The dynamical behaviors of both slow and fast
magnetosonic solitary waves is explored in detail. Exact accelerated
magnetosonic lump solutions are shown to be stable for the entire region in
parameter space of slow waves and a large region in parameter space of fast
waves. In a similar way, magnetosonic curved solitary waves become stable for a
small region in parameter space of fast waves. These exact solutions with
special properties are derived for specific choices of debris functions. These
novel results can have potential applications in scientific and technological
aspects of space debris detection and mitigation.
