All Stories

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