Showing 1–20 of 53 results
/ Date/ Name
Jan 25, 2022Statistical analysis of intermittency and its association with proton heating in the near Sun environmentDec 16, 2019Kinetic Scale Spectral Features of Cross Helicity and Residual Energy in the Inner HeliosphereDec 4, 2019Magnetic connectivity of the ecliptic plane within 0.5 AU : PFSS modeling of the first PSP encounterAug 19, 2021Ambipolar electric field and potential in the solar wind estimated from electron velocity distribution functionsFeb 5, 2021Determination of Solar Wind Angular Momentum and Alfvén Radius from Parker Solar Probe ObservationsSep 19, 2019Electron energy partition across interplanetary shocks: II. StatisticsNov 21, 2013Collisional Thermalization of Hydrogen and Helium in Solar Wind PlasmaMar 13, 2018ALPS: The Arbitrary Linear Plasma SolverFeb 23, 2018The statistical properties of solar wind temperature parameters near 1 AUFeb 26, 2025Helium Abundance Periods Observed by the Solar Probe Cup on Parker Solar Probe: Encounters 1-14Aug 12, 2025Observational Constraints on the Radial Evolution of O$^{6+}$ Temperature and Differential Flow in the Inner HeliosphereMar 11, 2026Strong Prevalence of Hammerhead Velocity Distributions Close to the Heliospheric Current SheetMar 8, 2023Prediction and Verification of Parker Solar Probe Solar Wind Sources at 13.3 R$_\odot$Oct 28, 2020Wave-particle energy transfer directly observed in an ion cyclotron waveSep 3, 2021Characteristic scales of magnetic switchback patches near the Sun and their possible association with solar supergranulation and granulationDec 9, 2019Proton Temperature Anisotropy Variations in Inner Heliosphere Estimated with First Parker Solar Probe ObservationsJan 10, 2020Density Fluctuations in the Solar Wind Based on Type III Radio Bursts Observed by Parker Solar ProbeSep 10, 2021Predicting the Magnetic Fields of a Stealth CME Detected by Parker Solar Probe at 0.5 AUAug 30, 2024In situ observations of large amplitude Alfvén waves heating and accelerating the solar windMay 15, 2024Calibrating the WSA model in EUHFORIA based on PSP observations