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Orlando Romeo
University of California BerkeleyMeeting roles in:
Understanding Spacecraft Surface Charging Effects with Simple Parker Solar Probe Models
Characterization of the Turbulence Properties of the Solar Wind as Observed by Parker Solar Probe in Encounters 8-19
Parker Solar Probe Observations of the Scaling of Plasma Heating by Magnetic Reconnection in the near-Sun Heliospheric Current Sheet
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
Heavy Ion Acceleration at 6 Solar Radii as Observed by Parker Solar Probe
In situ evidence of 5-minute oscillations from Parker Solar Probe
Cold Electron Distributions Observed by PSP During the March 13, 2023 CME
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
High-Frequency Solar Wind Electron Density Measurements Derived from Spacecraft Surface Charging Method on Parker Solar Probe
The FOXSI-4 Observation
Preflight Performance of the SupraThermal Ion Sensor (STIS) on the Space Weather Follow On-Lagrange 1 (SWFO-L1) Mission
Statistics of circularly polarized Type III storms
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