All Stories

  1. Non-Maxwellianity of ion velocity distributions in the Earth's magnetosheath
  2. Free Energy Source of the Mirror Instability: Nonresonant Particles
  3. Extending the wave telescope technique to larger numbers of spacecraft obtaining robust spatial power spectra
  4. Observational Constraints on the Radial Evolution of O6+ Temperature and Differential Flow in the Inner Heliosphere
  5. The dielectric response of plasmas with arbitrary gyrotropic velocity distributions
  6. Parker Solar Probe Observations of Turbulence and Waves between a Current Sheet and an Interplanetary Coronal Mass Ejection–Driven Shock
  7. A two-fluid solar-wind model with intermittent Alfvénic turbulence
  8. Impact of Two-population α-particle Distributions on Plasma Stability
  9. Identification of Ion-kinetic Instabilities in Hybrid-PIC Simulations of Solar Wind Plasma with Machine Learning
  10. Evidence of Interaction between Ion-scale Waves and Ion Velocity Distributions in the Solar Wind
  11. Quasithermal Noise in Magnetized Plasma: Theory and Simulations
  12. Nonlinear Interactions in Spherically Polarized Alfvénic Turbulence
  13. Modeling Hot, Anisotropic Ion Beams in the Solar Wind Motivated by the Parker Solar Probe Observations near Perihelia
  14. PLUME: Plasma in a Linear Uniform Magnetized Environment
  15. Solar Wind Electron Instabilities caused by Uneven Temperatures — Analyzed with ALPS
  16. Extreme Heating of Minor Ions in Imbalanced Solar-wind Turbulence
  17. Turbulent Energy Conversion Associated With Kinetic Microinstabilities in Earth's Magnetosheath
  18. Wave‐Telescope Analysis for Multipoint Observatories: Impact of Timing and Spatial Uncertainties
  19. Radial Evolution of Non-Maxwellian Electron Populations Derived from Quasi-thermal Noise Spectroscopy: Parker Solar Probe Observations
  20. Electron Influence on the Parallel Proton Firehose Instability in 10-moment, Multifluid Simulations
  21. Regulation of Solar Wind Electron Temperature Anisotropy by Collisions and Instabilities
  22. Measurement of the Taylor Microscale and the Effective Magnetic Reynolds Number in the Solar Wind With Cluster
  23. Wave-Telescope Analysis for Multipoint Observatories: Impact of Timing and Spatial Uncertainties
  24. Direct observation of ion cyclotron damping of turbulence in Earth’s magnetosheath plasma
  25. Estimated Heating Rates Due to Cyclotron Damping of Ion-scale Waves Observed by the Parker Solar Probe
  26. Evaluation of Scale-dependent Kurtosis with HelioSwarm
  27. Boundary of the Distribution of Solar Wind Proton Beta versus Temperature Anisotropy
  28. Constrained Wave-telescope Technique
  29. Erratum: “Parker Solar Probe Observations of High Plasma β Solar Wind from the Streamer Belt” (2023, ApJS, 265, 47)
  30. Parallel Diffusion Coefficient of Energetic Charged Particles in the Inner Heliosphere from the Turbulent Magnetic Fields Measured by Parker Solar Probe
  31. Analysis Techniques for Future Multipoint, Multiscale Observatories
  32. Mind the gap: Nonlocal cascades and preferential heating in high-β Alfvénic turbulence
  33. Zone of Preferential Heating for Minor Ions in the Solar Wind
  34. Multi‐Spacecraft Magnetic Field Reconstructions: A Cross‐Scale Comparison of Methods
  35. Collaborative Research: Vlasov‐Maxwell Simulations to Resolve Electron Heating and Dissipation, in Quasi‐Perpendicular Shocks
  36. Application of collisional analysis to the differential velocity of solar wind ions
  37. Proton- and Alpha-driven Instabilities in an Ion Cyclotron Wave Event
  38. Velocity-space Signatures of Resonant Energy Transfer between Whistler Waves and Electrons in the Earth’s Magnetosheath
  39. Erratum: “The Statistical Properties of Solar Wind Temperature Parameters Near 1 au” (2018, ApJS, 236, 41)
  40. Three-Dimensional Energy Transfer in Space Plasma Turbulence from Multipoint Measurement
  41. Analyses of ∼0.05–2 MeV Ions Associated with the 2022 February 16 Energetic Storm Particle Event Observed by Parker Solar Probe
  42. HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
  43. Corrigendum: Magnetic field reconstruction for a realistic multi-point, multi-scale spacecraft observatory
  44. The Effects of Nonequilibrium Velocity Distributions on Alfvén Ion-cyclotron Waves in the Solar Wind
  45. Near-Sun In Situ and Remote-sensing Observations of a Coronal Mass Ejection and its Effect on the Heliospheric Current Sheet
  46. Estimation of the error in the calculation of the pressure‐strain term: Application in the terrestrial magnetosphere
  47. Magnetospheric Multiscale measurements of turbulent electric fields in earth's magnetosheath: How do plasma conditions influence the balance of terms in generalized Ohm's law?
  48. Plasma turbulence: Challenges and next transformative steps from the perspective of multi-spacecraft measurements
  49. Intelligent Missions in the Living Heliospheric System Observatory
  50. Revolutionizing our Understanding of Particle Energization in Space Plasmas Using On-Board Wave-Particle Correlator Instrumentation
  51. HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
  52. Disentangling the Spatiotemporal Structure of Turbulence Using Multi-Spacecraft Data
  53. Enabling Discoveries in Heliospheric Science through Laboratory Plasma Experiments
  54. Firefly: The Case for a Holistic Understanding of the Global Structure and Dynamics of the Sun and the Heliosphere
  55. Next Generation Machine to Study Heliophysics in the Laboratory
  56. The Physics of Collisionless Dissipation in the Heliosphere
  57. Ion-driven Instabilities in the Inner Heliosphere. II. Classification and Multidimensional Mapping
  58. Quantifying the Energy Budget in the Solar Wind from 13.3 to 100 Solar Radii
  59. The Structure and Origin of Switchbacks: Parker Solar Probe Observations
  60. Anterograde Collisional Analysis of Solar Wind Ions
  61. Data-driven Uncertainty Quantification of the Wave Telescope Technique: General Equations and Demonstration Using HelioSwarm
  62. Estimation of the error on the calculation of the pressure-strain term: application in the terrestrial magnetosphere
  63. Estimation of Turbulent Proton and Electron Heating Rates via Landau Damping Constrained by Parker Solar Probe Observations
  64. Parker Solar Probe Observations of High Plasma β Solar Wind from the Streamer Belt
  65. Generalised Ohm’s Law in the Magnetosheath: How do plasma conditions impact turbulent electric fields?
  66. Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum
  67. Phase-space Energization of Ions in Oblique Shocks
  68. In Situ Signature of Cyclotron Resonant Heating in the Solar Wind
  69. The Solar Probe ANalyzer—Ions on the Parker Solar Probe
  70. Wind/Waves Antenna Length Determined Using Quasi-Thermal Noise Spectroscopy
  71. Patches of Magnetic Switchbacks and Their Origins
  72. Whistler Waves as a Signature of Converging Magnetic Holes in Space Plasmas
  73. Revolutionizing Our Understanding of Particle Energization in Space Plasmas Using On-Board Wave-Particle Correlator Instrumentation
  74. Plasma Parameters From Quasi‐Thermal Noise Observed by Parker Solar Probe: A New Model for the Antenna Response
  75. HelioSwarm: The Nature of Turbulence in Space Plasma
  76. Strong Perpendicular Velocity-space Diffusion in Proton Beams Observed by Parker Solar Probe
  77. Parker Solar Probe Enters the Magnetically Dominated Solar Corona
  78. Plasma Parameters from Quasi-Thermal Noise Observed by Parker Solar Probe: A New Model for the Antenna Response
  79. Ion-driven Instabilities in the Inner Heliosphere. I. Statistical Trends
  80. Plasma Waves in the Distant Martian Environment: Implications for Mars’ Sphere of Influence
  81. Experimental determination of ion acoustic wave dispersion relation with interferometric analysis
  82. Magnetic Field Reconstruction for a Realistic Multi-Point, Multi-Scale Spacecraft Observatory
  83. A Case for Electron-Astrophysics
  84. A field–particle correlation analysis of a perpendicular magnetized collisionless shock
  85. Detection of small magnetic flux ropes from the third and fourth Parker Solar Probe encounters
  86. Electron heat flux in the near-Sun environment
  87. The near-Sun streamer belt solar wind: turbulence and solar wind acceleration
  88. Wave-particle energy transfer directly observed in an ion cyclotron wave
  89. A powerful machine learning technique to extract proton core, beam, and alpha-particle parameters from velocity distribution functions in space plasmas
  90. Determining Threshold Instrumental Resolutions for Resolving the Velocity‐Space Signature of Ion Landau Damping
  91. PATCH: Particle Arrival Time Correlation for Heliophysics
  92. Multiscale Solar Wind Turbulence Properties inside and near Switchbacks Measured by the Parker Solar Probe
  93. How Alfvén waves energize the solar wind: heat versus work
  94. HelioSwarm: Leveraging Multi-Point, Multi-Scale Spacecraft Observations to Characterize Turbulence
  95. The Near-Sun Streamer Belt Solar Wind: Turbulence and Solar Wind Acceleration
  96. Inferred Linear Stability of Parker Solar Probe Observations Using One- and Two-component Proton Distributions
  97. Ion versus Electron Heating in Compressively Driven Astrophysical Gyrokinetic Turbulence
  98. Turbulence Characteristics of Switchback and Nonswitchback Intervals Observed by Parker Solar Probe
  99. Creation of large temperature anisotropies in a laboratory plasma
  100. Small-scale Magnetic Flux Ropes in the First Two Parker Solar Probe Encounters
  101. Proton core behaviour inside magnetic field switchbacks
  102. Diagnosing collisionless energy transfer using field–particle correlations: Alfvén-ion cyclotron turbulence
  103. Solar Wind Electron Parameters Determination on Wind Spacecraft Using Quasi‐Thermal Noise Spectroscopy
  104. The Heliospheric Current Sheet and Plasma Sheet during Parker Solar Probe’s First Orbit
  105. Parker Solar Probe Observations of Proton Beams Simultaneous with Ion-scale Waves
  106. Dependence of kinetic plasma waves on ion-to-electron mass ratio and light-to-Alfvén speed ratio
  107. The Solar Probe ANalyzers—Electrons on the Parker Solar Probe
  108. Proton Temperature Anisotropy Variations in Inner Heliosphere Estimated with the First Parker Solar Probe Observations
  109. Ion-scale Electromagnetic Waves in the Inner Heliosphere
  110. Kinetic-scale Spectral Features of Cross Helicity and Residual Energy in the Inner Heliosphere
  111. The Enhancement of Proton Stochastic Heating in the Near-Sun Solar Wind
  112. Electrons in the Young Solar Wind: First Results from the Parker Solar Probe
  113. Enhanced Energy Transfer Rate in Solar Wind Turbulence Observed near the Sun from Parker Solar Probe
  114. Identification of Magnetic Flux Ropes from Parker Solar Probe Observations during the First Encounter
  115. Magnetic Field Kinks and Folds in the Solar Wind
  116. Predicting the Solar Wind at the Parker Solar Probe Using an Empirically Driven MHD Model
  117. Sharp Alfvénic Impulses in the Near-Sun Solar Wind
  118. Solar Energetic Particles Produced by a Slow Coronal Mass Ejection at ∼0.25 au
  119. The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere
  120. The Solar Probe Cup on the Parker Solar Probe
  121. Turbulence Transport Modeling and First Orbit Parker Solar Probe (PSP) Observations
  122. Linear Stability in the Inner Heliosphere: Helios Re-evaluated
  123. The multi-scale nature of the solar wind
  124. Alfvénic velocity spikes and rotational flows in the near-Sun solar wind
  125. Solar Wind Temperature Isotropy
  126. Transition from ion-coupled to electron-only reconnection: Basic physics and implications for plasma turbulence
  127. Collisionless energy transfer in kinetic turbulence: field–particle correlations in Fourier space
  128. Solar Wind Plasma Parameter Distributions at 1 au
  129. Radial Evolution of Stochastic Heating in Low-β Solar Wind
  130. Strong Preferential Ion Heating is Limited to within the Solar Alfvén Surface
  131. Interplay between intermittency and dissipation in collisionless plasma turbulence
  132. Predictions for the First Parker Solar Probe Encounter
  133. Evidence for electron Landau damping in space plasma turbulence
  134. Stochastic proton heating by kinetic-Alfvén-wave turbulence in moderately high- plasmas
  135. Large-scale Control of Kinetic Dissipation in the Solar Wind
  136. ALPS: the Arbitrary Linear Plasma Solver
  137. The Statistical Properties of Solar Wind Temperature Parameters Near 1 au
  138. Majority of Solar Wind Intervals Support Ion-Driven Instabilities
  139. Astrophysical gyrokinetics: turbulence in pressure-anisotropic plasmas at ion scales and beyond
  140. Magnetic Reconnection May Control the Ion-scale Spectral Break of Solar Wind Turbulence
  141. Spatially localized particle energization by Landau damping in current sheets produced by strong Alfvén wave collisions
  142. Nonlinear energy transfer and current sheet development in localized Alfvén wavepacket collisions in the strong turbulence limit
  143. Nature of Stochastic Ion Heating in the Solar Wind: Testing the Dependence on Plasma Beta and Turbulence Amplitude
  144. A Zone of Preferential Ion Heating Extends Tens of Solar Radii from the Sun
  145. Applying Nyquist's method for stability determination to solar wind observations
  146. Diagnosing collisionless energy transfer using field–particle correlations: gyrokinetic turbulence
  147. Characterizing fluid and kinetic instabilities using field-particle correlations on single-point time series
  148. Diagnosing collisionless energy transfer using field–particle correlations: Vlasov–Poisson plasmas
  149. ENERGY DISSIPATION AND LANDAU DAMPING IN TWO- AND THREE-DIMENSIONAL PLASMA TURBULENCE
  150. COLLISIONLESS ISOTROPIZATION OF THE SOLAR-WIND PROTONS BY COMPRESSIVE FLUCTUATIONS AND PLASMA INSTABILITIES
  151. MEASURING COLLISIONLESS DAMPING IN HELIOSPHERIC PLASMAS USING FIELD–PARTICLE CORRELATIONS
  152. EVOLUTION OF THE PROTON VELOCITY DISTRIBUTION DUE TO STOCHASTIC HEATING IN THE NEAR-SUN SOLAR WIND
  153. ON THE CONSERVATION OF CROSS HELICITY AND WAVE ACTION IN SOLAR-WIND MODELS WITH NON-WKB ALFVÉN WAVE REFLECTION
  154. A MODIFIED VERSION OF TAYLOR’S HYPOTHESIS FOR SOLAR PROBE PLUS OBSERVATIONS
  155. Predicted impacts of proton temperature anisotropy on solar wind turbulence
  156. THE VIOLATION OF THE TAYLOR HYPOTHESIS IN MEASUREMENTS OF SOLAR WIND TURBULENCE
  157. VALIDITY OF THE TAYLOR HYPOTHESIS FOR LINEAR KINETIC WAVES IN THE WEAKLY COLLISIONAL SOLAR WIND
  158. PHYSICAL INTERPRETATION OF THE ANGLE-DEPENDENT MAGNETIC HELICITY SPECTRUM IN THE SOLAR WIND: THE NATURE OF TURBULENT FLUCTUATIONS NEAR THE PROTON GYRORADIUS SCALE
  159. Kinetic scale density fluctuations in the solar wind
  160. USING SYNTHETIC SPACECRAFT DATA TO INTERPRET COMPRESSIBLE FLUCTUATIONS IN SOLAR WIND TURBULENCE
  161. INTERPRETING MAGNETIC VARIANCE ANISOTROPY MEASUREMENTS IN THE SOLAR WIND
  162. THE SLOW-MODE NATURE OF COMPRESSIBLE WAVE POWER IN SOLAR WIND TURBULENCE