Weak double layers in the auroral ionosphere

Details Weak double layers in the auroral ionosphere Weak double layers in the auroral ionosphere

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nascp2469..225h&link_type=abstract

In NASA. Marshall Space Flight Center Double Layers in Astrophysics p 225-245 (SEE N87-23313 16-88)

Physics

Auroras, Earth Ionosphere, Electric Fields, Ion Acoustic Waves, Magnetohydrodynamic Stability, Plasma Layers, Plasmas (Physics), Boundary Value Problems, Electrostatics, Hydrogen Ions, Ion Density (Concentration), Oxygen Ions, Plasma Potentials

Scientific paper

Previous work on the evolution of weak double layers in a hydrogen plasma was extended to include H(+) and O(+) with relative drift. The relative drift between hydrogen and oxygen ions due to a quasi-static parallel electric field gives rise to a strong linear fluid instability which dominates the ion-acoustic mode at the bottom of the auroral acceleration region. This ion-ion instability can modify ion distributions at lower altitudes and the subsequent nonlinear evolution of weak double layers at higher altitudes in the ion-acoustic regime. Ion hole formation can occur for smaller relative electron-ion drifts than seen in previous simulations, due to the hydrogen-oxygen two-stream instability. This results in local modification of the ion distributions in phase space, and a partial filling of the valley between the hydrogen and oxygen peaks, which would be expected at higher altitudes on auroral field lines. The observed velocity diffusion does not necessarily preclude ion hole and double layer formation in hydrogen in the ion-acoustic regime. These simulation results are consistent with the experimentally measured persistence of separate hydrogen and oxygen peaks, and the observation of weak double layers above an altitude of 3000 km on auroral field lines.

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