Electron heat flux in the magnetosheath is shaped by magnetic field draping, increases with field strength, and is limited by whistler instability thresholds.
We use the highest-resolution burst-mode data to avoid effects of lossy compression of fast-mode data [42]
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Electron Heat Flux and Whistler Instability in the Earth's Magnetosheath
Electron heat flux in the magnetosheath is shaped by magnetic field draping, increases with field strength, and is limited by whistler instability thresholds.