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Magnetic Topology Effects on Energy Dissipation in Turbulent Plasma

ISSI Team led by Vyacheslav Olshevsky (BE) & Francesco Valentini (IT)

Magnetic Topology Effects on Energy Dissipation in Turbulent Plasma

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Publications

  1. O Marks the Spot for Magnetic Reconnection (2017)
  2. For Magnetic Reconnection Energy, O—not X—Might Mark the Spot (2017)
  3. Properties of Decaying Plasma Turbulence at Subproton Scales (2018)
  4. Detection of magnetic nulls around reconnection fronts (2018)
  5. Electron dynamics in magnetosheath mirror-mode structures (2018)
  6. Waves in Kinetic‐Scale Magnetic Dips: MMS Observations in the Magnetosheath (2018)
  7. Properties of Decaying Plasma Turbulence at Subproton Scales (2018)
  8. Evidence of magnetic nulls in electron diffusion region (2019)
  9. Electron distribution functions around a reconnection X-line resolved by the FOTE method (2019)
  10. Evidence of Radial Nulls Near Reconnection Fronts (2019)
  11. SOTE: A Nonlinear Method for Magnetic Topology Reconstruction in Space Plasmas (2019)
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