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Samuel Badman
Smithsonian Astrophysical ObservatoryMeeting roles in:
Following a Filament Eruption from the Sun to Earth that caused an Intense Geomagnetic Storm
Can We Predict the Solar Wind at Earth Using Parker Solar Probe Measurements?
PSP Observations of a Plasmoid Associated With Active Reconnection in the Near-Sun Heliospheric Current Sheet
Characterization of the Turbulence Properties of the Solar Wind as Observed by Parker Solar Probe in Encounters 8-19
Asymmetric Tangential Velocity inside Switchbacks: Implication for Switchback Origin
Energy Flux Contributions and Alfvénic Wave Dynamics in the Inner Heliosphere: Results from Parker Solar Probe Encounters 22–24
Ion-Scale Wave Properties Near the Heliospheric Current Sheet: A Parker Solar Probe–Wind Conjunction Study
Investigating hemispheric asymmetries in coronal hole solar wind structured by magnetolatitude
Direct Measurement of Polar Coronal Hole-like Solar Wind in its Acceleration Phase
Tracing the Radial Evolution of Solar Wind Streams Using Dynamic Time Warping: Multi-Spacecraft Observations by Parker Solar Probe, Solar Orbiter, and Wind
Heavy Ion Measurements in the Inner Heliosphere by the SPAN-I sensor
HelioSwitch: A High‑Purity Parker Solar Probe Switchback Catalog
In situ evidence of 5-minute oscillations from Parker Solar Probe
Quantifying Proton Heat Flux in Solar Wind Switchbacks Using a Gyrotropic Slepian Basis Reconstruction
Radial velocity fluctuations at Parker Solar Probe during closest approach in encounter 22
Solar Wind Angular Momentum Flux Calculated with Calibrated Transverse Velocity Measured by SPAN-Ion onboard Parker Solar Probe Mission During E22-E24
Quantification of Error in Potential Field Source Surface Modeling for Identification of the Source Regions of the Slow Alfvenic Solar Wind
Evolution of Alfvénic Magnetic Deflections and Energy Flux Densities from Sub- to Super-Alfvénic Solar Wind Environments
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