PIC simulations show E·B ≠ 0 regions reduce magnetic helicity in sub-ion turbulence, and a new history-dependent helicity density produces time-independent intermediate-scale plateaus consistent with cancellation-dominated 2D decay.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
roles
background 1polarities
background 1representative citing papers
Electron heat flux in the magnetosheath is shaped by magnetic field draping, increases with field strength, and is limited by whistler instability thresholds.
citing papers explorer
-
Kinetic Route to Helicity-Constrained Decay
PIC simulations show E·B ≠ 0 regions reduce magnetic helicity in sub-ion turbulence, and a new history-dependent helicity density produces time-independent intermediate-scale plateaus consistent with cancellation-dominated 2D decay.
-
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.