A wave-number-dependent closure for fluid moment equations is derived by mapping Padé approximant coefficients directly to the kinetic roots of the collisionless Vlasov-Poisson system, preserving the primary dispersion relation and extending to collisional plasmas.
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Electron heat flux in the magnetosheath is shaped by magnetic field draping, increases with field strength, and is limited by whistler instability thresholds.
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Wave-number-dependent closure condition for fluid moment equations
A wave-number-dependent closure for fluid moment equations is derived by mapping Padé approximant coefficients directly to the kinetic roots of the collisionless Vlasov-Poisson system, preserving the primary dispersion relation and extending to collisional plasmas.
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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.