Date of Award
Summer 6-2013
Access Type
Thesis - Open Access
Degree Name
Master of Science in Engineering Physics
Department
Physical Sciences
Committee Chair
Matthew Zettergren
First Committee Member
John M. Hughes
Second Committee Member
Jonathan B. Snively
Third Committee Member
Anatoly V. Streltsov
Abstract
A new 3-D model of the high latitude ionosphere is developed to study the coupling of the ionosphere with the magnetosphere and neutral atmosphere. The model consists of equations describing conservations of mass, momentum and energy for the six ionospheric constituents (O+, NO+, N+2 , O+2 , N+ and e-) and an electrostatic potential equation. This 3-D model is used to examine interrelated processes of ion heating, plasma structuring due to perpendicular transport, ion upflow, molecular ion generation, and neutral wave forcing. It is first validated by comparisons with a 2-D model, which uses similar mathematical and numerical approaches, and is additionally compared against incoherent scatter radar data. Results from a simulation of ionospheric response to a large amplitude acoustic wave also suggests an important role for these waves in generating local dynamo currents and density variations. Results of this model also shed some light on the interplay of perpendicular and parallel transports of plasma in producing structures in density and drift velocity profiles.
Scholarly Commons Citation
Lee, Yishi, "A 3-D Model of the Auroral Ionosphere" (2013). Doctoral Dissertations and Master's Theses. 90.
https://commons.erau.edu/edt/90
Included in
Oceanography and Atmospheric Sciences and Meteorology Commons, Plasma and Beam Physics Commons