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Francesco Pecora
University of DelawareMeeting roles in:
Reconstruction of Mesoscale Solar Wind Structures in Shear-Driven Turbulence
Correlation Scale Turbulence as the Driver of Magnetic Reconnection
Exploring Magnetic Island Morphology through 2D MHD and Synthetic Fields
Unravelling the link between turbulence, intermittency, and dissipation in the terrestrial magnetosheath
Turbulence 'Pressure Cooker' and Energization of Suprathermal Particles: IMAP, L1 Constellation, PSP and SO
Interplanetary magnetic correlation and low-frequency spectrum over many solar rotations
Scale Filtering Technique to Quantify Collisional Behavior in Collisionless Plasma
Scale-dependent Skewness and Kurtosis in Kinetic Plasmas and Magnetohydrodynamic Systems
Characterization of the Turbulence Properties of the Solar Wind as Observed by Parker Solar Probe in Encounters 8-19
The Effect of Turbulence on the Angular Momentum of the Solar Wind, measured via Parker Solar Probe Data and Global Modeling
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