MHD structures, waves and turbulence in the solar wind: Observations and theories

1995/07/01 by Chuanyi Tu, C. -Y. Tu, E. Marsch · 11 citations
Physics and Astronomy · Earth and Planetary Sciences · #Solar and Space Plasma Dynamics #Ionosphere and magnetosphere dynamics #Tropical and Extratropical Cyclones Research

paper · doi:10.1007/bf00748891

Citations

• Velocity Space Diffusion from Weak Plasma Turbulence in a Magnetic Field
• Inertial-Range Spectrum of Hydromagnetic Turbulence
• Dynamics of the Interplanetary Gas and Magnetic Fields.

Cited by

• Residual energy in weakly compressible turbulence with a mean guide field
• The influence of Parker spiral on the reflection-driven turbulence
• The Physical Origin of Periodic Density Structures in the Solar Wind: Coronal Streamers as Magnetohydrodynamic Resonators
• Significant Amplification of Turbulent Energy Dissipation through the Shock Transition at Mars
• The transition from slow to fast wind as observed in composition observations
• Numerical Demonstration of Kolmogorov Scaling in Magnetohydrodynamic Turbulence
• Observational Constraints on the Radial Evolution of O6+ Temperature and Differential Flow in the Inner Heliosphere
• The Solar Orbiter mission
• Observations of the fluctuations in Interplanetary Magnetic Field around L1 point during the solar transient events of 2024 with MAG payload onboard Aditya-L1 spacecraft
• Impact of solar magnetic field amplitude and geometry on cosmic rays diffusion coefficients in the inner heliosphere
• Transport of Particles in Strongly Turbulent 3D Magnetized Plasmas