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Lynn Wilson
NASA Goddard Space Flight CenterMeeting roles in:
Observations of >MeV particles observed at a weak interplanetary shock by Parker Solar Probe
Multi-point Analyses of Spatial Characteristics, Temporal Evolution, and Geo-effectiveness of Mesoscale Solar Wind Structures
Solar Wind Helium Abundance: A Fixed-Amplitude Solar Activity Indicator for Space Weather Forecasting
Compressive Structures in The Foreshock of Interplanetary Shocks
Remote Gyrosensing of the Earth's Bow Shock
Ion-Scale Wave Properties Near the Heliospheric Current Sheet: A Parker Solar Probe–Wind Conjunction Study
Electron and turbulence properties during sub-Alfvénic CME solar wind
Ion heating and acceleration in magnetic reconnection and current sheets in shock-driven turbulence
Identifying Shock-drift Acceleration at Quasiperpendicular Shocks: Simulations and MMS Observations
Energy partition at a collisionless supercritical quasi-parallel shock
On Electron Acceleration at Earth’s Foreshock
Interpretable Machine Learning for ICME Identification: Leveraging Solar Wind Helium Abundance, Compressibility, and Cross Helicity
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