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Published on: February 23, 2017
Eastward transients in the dayside ionosphere. II. A parallel-plate capacitorlike effect
Magnus F Ivarsen1, Jean-Pierre St-Maurice1, Glenn C Hussey1
1University of Saskatchewan, Department of Physics and Engineering Physics, Saskatoon, Saskatchewan, Canada.
Geospace storms can trigger eastward electric field bursts in the dayside ionosphere, linked to energetic particle precipitation and turbulent Hall currents. These findings challenge current models of cusp region electrodynamics.
Area of Science:
- Space Physics
- Atmospheric Science
- Geophysics
Background:
- Geospace storms significantly impact Earth's magnetosphere and ionosphere.
- Previous studies often interpret cusp region electrodynamics in terms of poleward-moving auroral forms.
Purpose of the Study:
- To investigate chorus-wave-driven energetic particle precipitation during a geospace storm.
- To analyze associated ionospheric phenomena, including electric field enhancements and turbulence.
- To contextualize these observations within dayside ionosphere dynamics and compare them with a similar event during a superstorm.
Main Methods:
- Observation of energetic particle precipitation on closed magnetic field lines.
- Radar detection of meter-scale turbulence and ionospheric electric field enhancements.
- Comparison of events from April 2023 and May 2024 geospace storms.
Main Results:
- Observed chorus-wave-driven energetic particle precipitation on closed magnetic field lines.
- Detected simultaneous ionospheric impact ionization and strong electric field enhancements.
- Identified fast, eastward-moving electric field structures equatorward of the ionospheric cusp in both events.
- Associated these structures with turbulent Hall currents, challenging existing cusp electrodynamics models.
Conclusions:
- Transient eastward electrodynamic bursts in the dayside ionosphere may be a common feature of geomagnetic storms.
- These bursts challenge conventional explanations focusing on poleward-moving forms.
- The findings suggest wave-particle interactions or proton precipitation contribute to these phenomena.
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