All Stories

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