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The response of plasma density to breaking inertial gravity wave in the lower regions of ionosphere
1. H. C. Aveiro, D. L. Hysell, R. G. Caton, K. M. Groves, J. Klenzing, R. F. Pfaff, R. Stoneback, and R. A. Heelis, J. Geophys. Res. 117, A03325, doi:10.1029/2011JA017077 (2012).
18. M. Kelley, The Earth's Ionosphere, Plasma Physics & Electrodynamics (International Geophysics), 2nd ed. (Academic Press, 2009), Vol. 96, 556 pp.
23. J. R. Taylor, Ph.D. thesis, University of California, San Diego, 2008.
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We present a three-dimensional numerical study for the E and lower F region ionosphere coupled with the neutral atmosphere dynamics. This model is developed based on a previous ionospheric model that examines the transport patterns of plasma density given a prescribed neutral atmospheric flow. Inclusion of neutral dynamics in the model allows us to examine the charge-neutral interactions over the full evolution cycle of an inertial gravity wave when the background flow spins up from rest, saturates and eventually breaks. Using Lagrangian analyses, we show the mixing patterns of the ionospheric responses and the formation of ionospheric layers. The corresponding plasma density in this flow develops complex wave structures and small-scale patches during the gravity wave breaking event.
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