All Stories

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