Showing 1–20 of 31 results
/ Date/ Name
Jan 25, 2023The Structure and Origin of Switchbacks: Parker Solar Probe ObservationsJun 28, 2012Using Synthetic Spacecraft Data to Interpret Compressible Fluctuations in Solar Wind TurbulenceFeb 8, 2019Predictions for the First Parker Solar Probe EncounterDec 5, 2019The Evolution and Role of Solar Wind Turbulence in the Inner HeliosphereDec 5, 2019Identification of Magnetic Flux Ropes from Parker Solar Probe Observations during the First EncounterOct 20, 2020Electron heat flux in the near-Sun environmentJan 26, 2021Inferred Linear Stability of Parker Solar Probe Observations using One- and Two-Component Proton DistributionsMay 3, 2012Interpreting Magnetic Variance Anisotropy Measurements in the Solar WindDec 6, 2019Enhanced Energy Transfer Rate in Solar Wind Turbulence Observed near the Sun from Parker Solar ProbeMar 13, 2019[Plasma 2020 Decadal] Disentangling the Spatiotemporal Structure of Turbulence Using Multi-Spacecraft DataMar 13, 2019[Plasma 2020 Decadal] Multipoint Measurements of the Solar Wind: A Proposed Advance for Studying Magnetized TurbulenceOct 17, 2021Strong perpendicular velocity-space in proton beams observed by Parker Solar ProbeMay 19, 2017Nonlinear energy transfer and current sheet development in localized Alfven wavepacket collisions in the strong turbulence limitDec 4, 2019Electrons in the Young Solar Wind: First Results from the Parker Solar ProbeOct 20, 2023Multi-Spacecraft Magnetic Field Reconstructions: A Cross-Scale Comparison of MethodsJan 6, 2023Parker Solar Probe: Four Years of Discoveries at Solar Cycle MinimumMay 22, 2023Quantifying the Energy Budget in the Solar Wind from 13.3-100 Solar RadiiOct 9, 2020Detection of small magnetic flux ropes from the third and fourth Parker Solar Probe encountersApr 6, 2020Parker Solar Probe observations of proton beams simultaneous with ion-scale wavesDec 5, 2019Predicting the Solar Wind at Parker Solar Probe Using an Empirically Driven MHD Model