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Ali Rahmati
University of California BerkeleyMeeting roles in:
MAVEN’s Comprehensive Solar Flare Catalog for Mars: A Resource for Quantifying Solar Influence on Atmospheric Loss
Ion-Scale Wave Emission and Absorption from non-Maxwellian Velocity Distributions Measured by SWEAP/SPANi
The Solar Energetic Particle Detector on MAVEN: Bonus Science at Mars
Toward Safer Mars Missions: Space Weather Lessons from a Multipoint Observation Campaign
The MAVEN Space Weather Catalogue at Mars: Characterizing Solar Transient Events at 1.5 AU Over a Full Solar Cycle
Measuring high energy (10 MeV - 10 GeV) particles at Mars with the MAVEN Solar Energetic Particle detector, with a focus on Galactic Cosmic Ray modulation throughout the solar cycle (2015-2024).
Can We Predict the Solar Wind at Earth Using Parker Solar Probe Measurements?
Statistical Distributions of Elsasser Variables in the Near Sun Environment
Building a solar energetic particle event catalog for Mars
Solar electron events at Mars and solar radio bursts: Cross-mission study of MAVEN, Parker Solar Probe, and STEREO
Energy Flux Contributions and Alfvénic Wave Dynamics in the Inner Heliosphere: Results from Parker Solar Probe Encounters 22–24
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
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
Preflight Performance of the SupraThermal Ion Sensor (STIS) on the Space Weather Follow On-Lagrange 1 (SWFO-L1) Mission
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