All Stories

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