Revisiting Mars' Induced Magnetic Field and Clock Angle Departures under Real-Time Upstream Solar Wind Conditions

Documenti analoghi

• Magnetic Field and Plasma Asymmetries Between the Martian Quasi-Perpendicular and Quasi-Parallel Magnetosheaths
  di: Tadlock, Abigail, et al.
  Pubblicazione: (2025)
• Physics-Informed Neural Networks for Modeling the Martian Induced Magnetosphere
  di: Gao, Jiawei, et al.
  Pubblicazione: (2025)
• Properties and Radial Evolution of Solar Wind Turbulence Near Mercury's Orbit
  di: Li, Xinmin, et al.
  Pubblicazione: (2026)
• Automated Classification of Plasma Regions at Mars Using Machine Learning
  di: Qin, Yilan, et al.
  Pubblicazione: (2026)
• The Incompressible Magnetohydrodynamic Energy Cascade Rate Upstream of Mars: Effects of the Total Energy and the Cross-Helicity on Solar Wind Turbulence
  di: Romanelli, Norberto, et al.
  Pubblicazione: (2024)