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Phyllis Whittlesey
University of California Berkeley, Space Sciences LaboratoryMeeting roles in:
ESCAPADE's New Mission: Two-Point Space Weather Measurements at Earth, Mars, and in-Between
Can We Predict the Solar Wind at Earth Using Parker Solar Probe Measurements?
Overview of ESCAPADE Science Data Products for Two-Point Space Weather Measurements En Route to Mars
Energy Flux Contributions and Alfvénic Wave Dynamics in the Inner Heliosphere: Results from Parker Solar Probe Encounters 22–24
Observational evidence for suppression of magnetic reconnection by shear flow
Investigating hemispheric asymmetries in coronal hole solar wind structured by magnetolatitude
Direct Measurement of Polar Coronal Hole-like Solar Wind in its Acceleration Phase
Heavy Ion Measurements in the Inner Heliosphere by the SPAN-I sensor
Characterizing Pristine Solar Wind Thermodynamics Near the Sun Using Parker Solar Probe Observations from Encounters 22 to 24
Alpha Particle Temperature and Velocity Statistics in the Young Solar Wind
Cold Electron Distributions Observed by PSP During the March 13, 2023 CME
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
Electrons in the Collisionally Young Solar Wind: Parker Solar Probe Observations
High-Frequency Solar Wind Electron Density Measurements Derived from Spacecraft Surface Charging Method on Parker Solar Probe
Latitudinal structure of the heliospheric magnetic field and solar wind in the inner heliosphere: results of the first Solar Orbiter out of ecliptic orbit
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