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arXiv · 2004.11755

Mode Converting Alfv\'{e}n Waves from Magnetic Reconnection Enhancing the Energy Source for the Aurora Borealis

Harsha Gurram·Jan Egedal·William Daughton
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Abstract

Previous studies have concluded that the Hall magnetic field structures generated during magnetic reconnection are carried away by kinetic Alfv\'{e}n waves (KAW). Here we apply a kinetic simulation with an ion/electron mass ratio closer to its natural value and find that much-reduced damping rates permit the KAW to convert into shear Alfv\'{e}n waves (SAW). For magnetotail reconnection these SAW provides efficient transport of wave energy, enhancing the energy input for the Aurora Borealis by orders of magnitude above previous estimates.

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Harsha Gurram, Jan Egedal, William Daughton. 2020-04-24. Mode Converting Alfv\'{e}n Waves from Magnetic Reconnection Enhancing the Energy Source for the Aurora Borealis. https://arxiv.org/abs/2004.11755

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