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- W1628674423 abstract "The plasma convection in the inner magnetosphere reacts quickly after a growth of the polar cap potential, as revealed by the quick onset of the development of the partial ring current as demonstrated by Hashimoto et al. [2002]. In order to explain the quick response of the inner magnetosphere, we apply the Earth-ionosphere waveguide (transmission line) model developed by Kikuchi and Araki [ 979b]. In this paper, we examine how the TMO mode is excited in the waveguide by the electric potential transported along with the field-aligned currents, and show that the electric potential is transmitted horizontally at the speed of light in the Earth-ionosphere waveguide. We then evaluate the attenuation of the TMO mode by calculating the Poynting flux transported upward from the Earth-ionosphere waveguide into the conducting ionosphere. A fraction of the Poynting flux is further transported into the magnetosphere when the Alfven conductance of the magnetosphere is not very small compared with the ionospheric conductance. The upward transportation of the Poynting flux causes a loss of the horizontally transmitting energy, resulting in the attenuation of the TMO mode, but it is not substantial compared to the geometrical attenuation due to the finite size of the polar electric field. We stress that the electric field associated with the ionospheric current is mapped upward into the magnetosphere by the Alfven mode, which drives the plasma convection in the inner magnetosphere. We note that the ionosphere is not a generator but constitutes a transmission line for the electromagnetic energy to be transported into the inner magnetosphere." @default.
- W1628674423 created "2016-06-24" @default.
- W1628674423 creator A5054691687 @default.
- W1628674423 date "2013-03-18" @default.
- W1628674423 modified "2023-10-18" @default.
- W1628674423 title "Transmission Line Model for Driving Plasma Convection in the Inner Magnetosphere" @default.
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- W1628674423 doi "https://doi.org/10.1029/155gm20" @default.
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