Research Motivation
Space plasmas constitute more than 99% of the visible matter in the Universe, yet many of the fundamental processes governing their behavior remain poorly understood. My research seeks to uncover how energy is transferred, dissipated, and converted in collisionless plasmas, with particular emphasis on the physical processes that shape the heliosphere and drive space weather.
Space plasmas constitute more than 99% of the visible matter in the Universe, yet many of the fundamental processes governing their behavior remain poorly understood. My research seeks to uncover how energy is transferred, dissipated, and converted in collisionless plasmas, with particular emphasis on the physical processes that shape the heliosphere and drive space weather.
Solar eruptions, including coronal mass ejections (CMEs) and corotating interaction regions (CIRs), continuously modify the near-Earth space environment and influence planetary magnetospheres, energetic particles, and cosmic rays. Understanding the plasma processes operating within these structures is essential for improving our ability to predict space weather and for advancing our knowledge of fundamental plasma physics.
Solar eruptions, including coronal mass ejections (CMEs) and corotating interaction regions (CIRs), continuously modify the near-Earth space environment and influence planetary magnetospheres, energetic particles, and cosmic rays. Understanding the plasma processes operating within these structures is essential for improving our ability to predict space weather and for advancing our knowledge of fundamental plasma physics.
My work combines spacecraft observations, plasma theory, and advanced data analysis to investigate plasma behavior across a wide range of spatial and temporal scales. I utilize measurements from missions such as Parker Solar Probe, Solar Orbiter, MMS, Wind, ACE, and Helios to study turbulence, current sheets, plasma waves, shocks, magnetic holes, temperature anisotropy, kinetic instabilities, and wave-particle interactions.
My work combines spacecraft observations, plasma theory, and advanced data analysis to investigate plasma behavior across a wide range of spatial and temporal scales. I utilize measurements from missions such as Parker Solar Probe, Solar Orbiter, MMS, Wind, ACE, and Helios to study turbulence, current sheets, plasma waves, shocks, magnetic holes, temperature anisotropy, kinetic instabilities, and wave-particle interactions.
A central goal of my research is to understand how microscopic plasma processes regulate large-scale dynamics, particle acceleration, plasma heating, and energy transport throughout the heliosphere. By bridging observations and theory, I aim to contribute to a more complete understanding of plasma processes in both heliospheric and astrophysical environments.
A central goal of my research is to understand how microscopic plasma processes regulate large-scale dynamics, particle acceleration, plasma heating, and energy transport throughout the heliosphere. By bridging observations and theory, I aim to contribute to a more complete understanding of plasma processes in both heliospheric and astrophysical environments.
