All Stories

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