All Stories

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