All Stories

  1. A Unified Three-dimensional Magnetohydrodynamic Model of the Solar Corona, Solar Wind, and Global Heliosphere with Turbulence Transport
  2. The Alfvén transition zone observed by the Parker Solar Probe in young solar wind – global properties and model comparisons
  3. Rayleigh‐Taylor Instability Observed at the Dayside Magnetopause Under Northward Interplanetary Magnetic Field
  4. Generalized Fluid Models of the Braginskii Type
  5. An extended and fragmented Alfvén zone in the Young Solar Wind
  6. Substructure of a Kelvin‐Helmholtz Vortex Accompanied by Plasma Transport Under the Northward Interplanetary Magnetic Field
  7. Large-scale Structure and Turbulence Transport in the Inner Solar Wind: Comparison of Parker Solar Probe’s First Five Orbits with a Global 3D Reynolds-averaged MHD Model
  8. Cluster After 20 Years of Operations: Science Highlights and Technical Challenges
  9. Random Walk and Trapping of Interplanetary Magnetic Field Lines: Global Simulation, Magnetic Connectivity, and Implications for Solar Energetic Particles
  10. The interpretation of data from the Parker Solar Probe mission: shear-driven transition to an isotropically turbulent solar wind
  11. Shear-driven Transition to Isotropically Turbulent Solar Wind Outside the Alfvén Critical Zone
  12. Enhanced Energy Transfer Rate in Solar Wind Turbulence Observed near the Sun from Parker Solar Probe
  13. Clustering of Intermittent Magnetic and Flow Structures near Parker Solar Probe’s First Perihelion—A Partial-variance-of-increments Analysis
  14. Measures of Scale-dependent Alfvénicity in the First PSP Solar Encounter
  15. Observations of Energetic-particle Population Enhancements along Intermittent Structures near the Sun from the Parker Solar Probe
  16. Observations of Heating along Intermittent Structures in the Inner Heliosphere from PSP Data
  17. The Solar Wind Electron Halo as Produced by Electron Beams Originating in Nanoflares: Beam Density Dependence
  18. An introductory guide to fluid models with anisotropic temperatures. Part 1. CGL description and collisionless fluid hierarchy
  19. An introductory guide to fluid models with anisotropic temperatures. Part 2. Kinetic theory, Padé approximants and Landau fluid closures
  20. The Solar Wind Electron Halo as Produced by Electron Beams Originating in the Lower Corona: Beam Density Dependence
  21. Electron Vorticity Indicative of the Electron Diffusion Region of Magnetic Reconnection
  22. Contextual Predictions for Parker Solar Probe. II. Turbulence Properties and Taylor Hypothesis
  23. Contextual Predictions for the Parker Solar Probe. I. Critical Surfaces and Regions
  24. Structure and Dynamics of Three-Dimensional Magnetotail Reconnection
  25. The Steady Global Corona and Solar Wind: A Three-dimensional MHD Simulation with Turbulence Transport and Heating
  26. Weakened Magnetization and Onset of Large-scale Turbulence in the Young Solar Wind—Comparisons of Remote Sensing Observations with Simulation
  27. Magnetospheric Multiscale Observations of an Ion Diffusion Region With Large Guide Field at the Magnetopause: Current System, Electron Heating, and Plasma Waves
  28. Energy partitioning constraints at kinetic scales in low-βturbulence
  29. Multipoint observations of plasma phenomena made in space by Cluster
  30. Solar Cycle Occurrence of Alfvénic Fluctuations and Related Geo-Efficiency
  31. Erratum: “Electromagnetic Waves near the Proton Cyclotron Frequency: STEREO Observations” (2014, ApJ, 786, 123)
  32. Cosmic-Ray Diffusion Coefficients throughout the Inner Heliosphere from a Global Solar Wind Simulation
  33. Partitioning of integrated energy fluxes in four tail reconnection events observed by Cluster
  34. SOLAR WIND COLLISIONAL AGE FROM A GLOBAL MAGNETOHYDRODYNAMICS SIMULATION
  35. Effect of magnetic islands on the localization of kinetic Alfvén wave
  36. Kinetic scale turbulence and dissipation in the solar wind: key observational results and future outlook
  37. Multipoint observations of plasma phenomena made in space by Cluster
  38. Mission Oriented Support and Theory (MOST) for MMS—the Goddard Space Flight Center/University of California Los Angeles Interdisciplinary Science Program
  39. PICKUP ION MEDIATED PLASMAS. I. BASIC MODEL AND LINEAR WAVES IN THE SOLAR WIND AND LOCAL INTERSTELLAR MEDIUM
  40. THE ORIGIN OF NON-MAXWELLIAN SOLAR WIND ELECTRON VELOCITY DISTRIBUTION FUNCTION: CONNECTION TO NANOFLARES IN THE SOLAR CORONA
  41. RELAXATION PROCESSES IN SOLAR WIND TURBULENCE
  42. THREE-FLUID, THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC SOLAR WIND MODEL WITH EDDY VISCOSITY AND TURBULENT RESISTIVITY
  43. Open boundary particle-in-cell simulation of dipolarization front propagation
  44. Dipolarization and turbulence in the plasma sheet during a substorm: THEMIS observations and global MHD simulations
  45. Direct auroral precipitation from the magnetotail during substorms
  46. Numerical Simulation of Interplanetary and Magnetospheric Phenomena: The Kelvin-Helmholtz Instability
  47. Adiabatic acceleration of suprathermal electrons associated with dipolarization fronts
  48. THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC MODELING OF THE SOLAR WIND INCLUDING PICKUP PROTONS AND TURBULENCE TRANSPORT
  49. Vlasov simulation of electrostatic solitary structures in multi-component plasmas
  50. SCALE DEPENDENCE OF MAGNETIC HELICITY IN THE SOLAR WIND
  51. Correction to “Global magnetohydrodynamic simulation of reconnection and turbulence in the plasma sheet”
  52. Observation and theoretical modeling of electron scale solar wind turbulence
  53. Observations and simulations of non-local acceleration of electrons in magnetotail magnetic reconnection events
  54. SOLAR WIND MODELING WITH TURBULENCE TRANSPORT AND HEATING
  55. Global magnetohydrodynamic simulation of reconnection and turbulence in the plasma sheet
  56. Observations and Modeling of Turbulence in the Solar Wind
  57. Spectra of polar heliospheric fields and implications for field structure
  58. The first cluster and double star symposium
  59. Magnetospheric physics: Turbulence on a small scale
  60. NUMERICAL SIMULATIONS OF SOLAR WIND TURBULENCE
  61. An MHD Model for Heliospheric Studies
  62. A view of the inner heliosphere during the May 10-11, 1999 low density anomaly
  63. A global MHD solar wind model with WKB Alfvén waves: Comparison with Ulysses data
  64. Radio Astronomy at Long Wavelengths
  65. Preface
  66. Magnetohydrodynamic turbulence in the solar wind
  67. Erratum: Quasi-Two-Dimensional MHD Turbulence in Three-Dimensional Flows [Phys. Rev. Lett. 82, 548 (1999)]
  68. Quasi-Two-Dimensional MHD Turbulence in Three-Dimensional Flows
  69. A Vlasov moment description of cyclotron wave–particle interactions
  70. Nonlinear evolution of interplanetary Alfvénic fluctuations with convected structures
  71. Comments on “Alfvénic disturbances in the equatorial solar wind with a spiral magnetic field” by Yu-Qing Lou
  72. Magnetohydrodynamic turbulence and its relationship to interplanetary magnetic fluctuations
  73. On interacting plasma vortex sheets
  74. Quasi-periodic transverse plasma flow associated with an evolving MHD vortex street in the outer heliosphere
  75. An evolving MHD vortex street model for quasi-periodic solar wind fluctuations
  76. Velocity shear generation of solar wind turbulence
  77. Magnetohydrodynamic simulation of the radial evolution and stream structure of solar-wind turbulence
  78. Whistler waves associated with the Uranian bow shock: Outbound observations
  79. Parametric instabilities of circularly polarized large-amplitude dispersive Alfvén waves: excitation of parallel-propagating electromagnetic daughter waves
  80. Parametric instabilities of circularly polarized large-amplitude dispersive Alfvén waves: excitation of obliquely-propagating daughter and side-band waves
  81. Reply [to “Comment on ‘Do interplanetary Alfvén waves cause auroral activity?’ by D. Aaron Roberts and Melvyn L. Goldstein”]
  82. Anisotropy and minimum variance directions of solar wind fluctuations in the outer heliosphere
  83. Do interplanetary Alfvén waves cause auroral activity?
  84. Evidence for the presence of quasi-two-dimensional nearly incompressible fluctuations in the solar wind
  85. TURBULENT RELAXATION IN COMPRESSIBLE TWO-DIMENSIONAL MAGNETOHYDRODYNAMICS
  86. QUASI-TWO-DIMENSIONAL NEARLY-INCOMPRESSIBLE SOLAR WIND FLUCTUATIONS
  87. Whistler wave bursts upstream of the Uranian bow shock
  88. Spectral evolution and cascade constant of solar wind Alfvénic turbulence
  89. OBSERVATION AND SIMULATION OF MHD TURBULENCE IN THE SOLAR WIND
  90. Test particle acceleration in turbulent reconnecting magnetic fields
  91. Beam-driven ion cyclotron harmonic resonances in the terrestrial foreshock
  92. Large-amplitude MHD waves upstream of the Jovian bow shock: Reinterpretation
  93. Erratum: ‘‘Electromagnetic ion beam instabilities’’ [Phys. Fluids 27, 1852 (1984)]
  94. Spectral analysis of magnetohydrodynamic fluctuations near interplanetary shocks
  95. Electromagnetic ion beam instabilities
  96. Correction to “Turbulence analysis of the Jovian upstream ‘wave’ phenomenon”
  97. Correction to “Large amplitude MHD waves upstream of the Jovian bow shock”
  98. Turbulent Generation of Outward-Traveling Interplanetary Alfvénic Fluctuations
  99. Theories of radio emissions and plasma waves
  100. A theory of the Io phase asymmetry of the Jovian decametric radiation
  101. Turbulence analysis of the Jovian upstream ‘wave’ phenomenon
  102. Large amplitude MHD waves upstream of the Jovian bow shock
  103. Evaluation of Magnetic Helicity in Homogeneous Turbulence
  104. Stationarity of magnetohydrodynamic fluctuations in the solar wind
  105. Measurement of the rugged invariants of magnetohydrodynamic turbulence in the solar wind
  106. The formation of arcs in the dynamic spectra of Jovian decameter bursts
  107. The mean free path of low-rigidity cosmic rays
  108. Microscale instabilities in stream interaction regions
  109. A Theory of Solar Type III Radio Bursts
  110. Consequences of using nonlinear particle trajectories to compute spatial diffusion coefficients
  111. On the theory of the type III burst exciter
  112. Lunar magnetism
  113. Stabilization of Electron Streams in Type III Solar Radio Bursts
  114. Turbulent Heating of Colliding Streams in the Solar Wind
  115. The Plasma Physics of the Jovian Decameter Radiation
  116. The Theory of Inverse Compton Scattering in a Cold Plasma