All Stories

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