Turbulence

Turbulence in the solar wind is a key driver of plasma dynamics, transferring energy from large-scale structures to smaller scales where it can heat particles and accelerate them. This process is not uniform; it depends on factors like wind speed, magnetic field alignment, and distance from the Sun. By studying wave-particle interactions and the intermittent nature of turbulent fluctuations, we can better understand how the solar wind evolves as it travels through the heliosphere and what that means for predicting its impact on planetary environments.

Summary generated with ChatGPT based on my first-author publications for clarity and accessibility.