Observation of Discrete Harmonic Modes and Binary Scaling in High-Beta Solar Wind Turbulence

Key Points

• The aim is to explore the stability of magnetic structures in solar wind and their fit with fluid models.
• Observation of turbulent structures in near-Sun solar wind.
• Analysis of stability in magnetic switchbacks.
• Exploration of dimensionless parameters affecting these structures.
• Identification of discrete harmonic modes in solar wind turbulence.
• Evidence of binary scaling in turbulent structures.
• Challenge to the existing continuous fluid models.