All Stories

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