Birkeland current: Difference between revisions
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[[File:600px-Schematic-of-combined-FACs-and-ionospheric-current-systems.png|thumb|Schematic of the Birkeland or Field-Aligned Currents and the ionospheric current systems they connect to] | [[File:600px-Schematic-of-combined-FACs-and-ionospheric-current-systems.png|thumb|Schematic of the Birkeland or Field-Aligned Currents and the ionospheric current systems they connect to]] | ||
A [[Birkeland current]] is a set of currents that flow along geomagnetic field lines connecting the Earth’s [[Magnetosphere]] to the Earth's high latitude ionosphere. In the Earth’s magnetosphere, the currents are driven by the solar wind and interplanetary magnetic field and by bulk motions of plasma through the magnetosphere (convection indirectly driven by the interplanetary environment). The strength of the Birkeland currents changes with activity in the magnetosphere (e.g. during substorms). | A [[Birkeland current]] is a set of currents that flow along geomagnetic field lines connecting the Earth’s [[Magnetosphere]] to the Earth's high latitude ionosphere. In the Earth’s magnetosphere, the currents are driven by the solar wind and interplanetary magnetic field and by bulk motions of plasma through the magnetosphere (convection indirectly driven by the interplanetary environment). The strength of the Birkeland currents changes with activity in the magnetosphere (e.g. during substorms). | ||
Revision as of 22:58, 27 January 2016
A Birkeland current is a set of currents that flow along geomagnetic field lines connecting the Earth’s Magnetosphere to the Earth's high latitude ionosphere. In the Earth’s magnetosphere, the currents are driven by the solar wind and interplanetary magnetic field and by bulk motions of plasma through the magnetosphere (convection indirectly driven by the interplanetary environment). The strength of the Birkeland currents changes with activity in the magnetosphere (e.g. during substorms).
Small scale variations in the upward current sheets (downward flowing electrons) accelerate magnetospheric electrons which, when they reach the upper atmosphere, create the Auroras Borealis and Australis. In the high latitude ionosphere (or auroral zones), the Birkeland currents close through the region of the auroral electrojet, which flows perpendicular to the local magnetic field in the ionosphere. The Birkeland currents occur in two pairs of field-aligned current sheets.
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