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Energy Transport and Conversion Above a Bright Discrete Auroral Arc
1Space Sciences Laboratory University of California Berkeley CA USA.
Summary
Energy transport into discrete auroral arcs is facilitated by vortex formation and Poynting flux divergence. This convergence of energy powers observed electron acceleration in the magnetosphere.
Area of Science:
- Space Physics
- Magnetospheric Physics
- Plasma Physics
Background:
- Discrete auroral arcs are visual manifestations of energy transfer processes in Earth's magnetosphere.
- Understanding energy transport mechanisms is crucial for explaining particle acceleration phenomena.
Purpose of the Study:
- To investigate energy transport and conversion above a discrete auroral arc.
- To determine how energy converges into the acceleration region and powers electron energization.
Main Methods:
- Utilizing magnetically connected observations from the Reimei spacecraft.
- Combining in situ measurements of particle distributions and luminosity with imaging data.
- Analyzing transverse electromagnetic and kinetic energy fluxes along the spacecraft trajectory.
Main Results:
- Observed convergence of transverse energy fluxes into the acceleration region.
- Demonstrated facilitation of cross-field energy transport by vortex formation along the arc.
- Quantified energy inflow supporting local dissipation and electron acceleration.
Conclusions:
- Transverse and field-aligned energy flows into the arc locally support observed electron acceleration.
- Divergence of Poynting flux along and across the magnetic field drives field-aligned electron energization.
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