The early time evolution of an ionospheric electron depletion produced
by a radially expanding electron attachment chemical release is studi
ed with a two-dimensional simulation model. The model includes electro
n attachment chemistry, incorporates fluid electrons, particle ions an
d neutrals, and considers the evolution in a plane perpendicular to th
e geomagnetic field for a low beta plasma. Timescales considered are o
f the order of or less than the cyclotron period of the negative ions
that result as a by-product of the electron attachment reaction. This
corresponds to time periods of tenths of seconds during recent experim
ents. Simulation results show that a highly sheared azimuthal electron
flow velocity develops in the radially expanding depletion boundary.
This sheared electron flow velocity and the steep density gradients in
the boundary give rise to small-scale irregularities in the form of e
lectron density cavities and spikes. The nonlinear evolution of these
irregularities results in trapping and ultimately turbulent heating of
the negative ions.