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Published on: November 21, 2019
Magnetosphere sawtooth oscillations induced by ionospheric outflow
O J Brambles1, W Lotko, B Zhang
1Thayer School of Engineering, Dartmouth College, Hanover, NH, USA. ojbrambles@dartmouth.edu
Summary
Earth's magnetosphere exhibits sawtooth oscillations, driven by solar wind interactions. Ionospheric O(+) outflows are key, ejecting plasma and causing magnetic field changes.
Area of Science:
- Space Physics
- Geophysics
- Plasma Physics
Background:
- Earth's magnetosphere exhibits periodic sawtooth oscillations.
- These oscillations are planetary-scale and occur every 2-4 hours.
- The solar wind-magnetosphere-ionosphere (SW-M-I) interaction powers these oscillations.
Purpose of the Study:
- Investigate the role of ionospheric O(+) outflows in generating sawtooth oscillations.
- Understand the mechanisms driving the magnetospheric dynamics during these events.
Main Methods:
- Utilized global simulations of geospace.
- Analyzed the impact of ionospheric O(+) outflows on the inner magnetosphere.
Main Results:
- Ionospheric O(+) outflows were identified as a generator of sawtooth oscillations.
- Outflowing ions increase pressure, distending the nightside magnetic field.
- Exceeding an outflow threshold leads to plasmoid ejection and magnetic field dipolarization.
Conclusions:
- Ionospheric O(+) outflows are crucial for sawtooth oscillation generation.
- The SW-M-I interaction strength controls outflow fluence and oscillation period.
- Magnetospheric dynamics shift between quasi-steady convection and dynamic ejection events.
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