All Stories

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