All Stories

  1. Separate Exact Laws of Kinetic and Magnetic Energy Cascade in Magnetohydrodynamic Turbulence
  2. Particle Transport from First Principles in the Early Heliosphere: κ 1 Ceti as a Case Study for the Young Sun
  3. Direct power spectral density estimation from structure functions without Fourier transforms
  4. Factors controlling the statistics of magnetic reconnection in magnetohydrodynamic turbulence
  5. Finite Reynolds number effect on substantial inertial range in incompressible magnetohydrodynamic turbulence
  6. Estimation of Effective Viscosity to Quantify Collisional Behavior in Collisionless Plasma
  7. Magnetohydrodynamic turbulence and the associated spatial diffusion tensor of cosmic rays in dynamical galactic halos
  8. Measuring the turbulent energy cascade rate with multiple spacecraft
  9. Constraining Solar Wind Transport Model Parameters Using Bayesian Analysis
  10. Energy flux decomposition in magnetohydrodynamic turbulence
  11. What is the Reynolds Number of the Solar Wind?
  12. A Three-dimensional Model for the Evolution of Magnetohydrodynamic Turbulence in the Outer Heliosphere
  13. New exact Betchov-like relation for the helicity flux in homogeneous turbulence
  14. Strategies for Determining the Cascade Rate in MHD Turbulence: Isotropy, Anisotropy, and Spacecraft Sampling
  15. Turbulence in the Outer Heliosphere
  16. On the Generation of Compressible Mirror-mode Fluctuations in the Inner Heliosheath
  17. Critical Balance and the Physics of Magnetohydrodynamic Turbulence
  18. A detailed examination of anisotropy and timescales in three-dimensional incompressible magnetohydrodynamic turbulence
  19. Evolution of similarity lengths in anisotropic magnetohydrodynamic turbulence
  20. Reduced MHD in Astrophysical Applications: Two-dimensional or Three-dimensional?
  21. A GENERALIZED TWO-COMPONENT MODEL OF SOLAR WIND TURBULENCE AND AB INITIO DIFFUSION MEAN-FREE PATHS AND DRIFT LENGTHSCALES OF COSMIC RAYS
  22. VARIANCE ANISOTROPY IN KINETIC PLASMAS
  23. Variance anisotropy in compressible 3-D MHD
  24. Intermittency, nonlinear dynamics and dissipation in the solar wind and astrophysical plasmas
  25. Anisotropy in solar wind plasma turbulence
  26. DISSIPATION AND RECONNECTION IN BOUNDARY-DRIVEN REDUCED MAGNETOHYDRODYNAMICS
  27. NONLINEAR AND LINEAR TIMESCALES NEAR KINETIC SCALES IN SOLAR WIND TURBULENCE
  28. COMPLEXITY AND DIFFUSION OF MAGNETIC FLUX SURFACES IN ANISOTROPIC TURBULENCE
  29. MAGNETIC FIELD LINE RANDOM WALK IN MODELS AND SIMULATIONS OF REDUCED MAGNETOHYDRODYNAMIC TURBULENCE
  30. ON THE ORIGIN OF ANISOTROPY IN MAGNETOHYDRODYNAMIC TURBULENCE: THE ROLE OF HIGHER-ORDER CORRELATIONS
  31. Generation of X-points and secondary islands in 2D magnetohydrodynamic turbulence
  32. Solar wind fluctuations and the von Kármán–Howarth equations: The role of fourth-order correlations
  33. Scaling anisotropy of the power in parallel and perpendicular components of the solar wind magnetic field
  34. LOCAL ANISOTROPY, HIGHER ORDER STATISTICS, AND TURBULENCE SPECTRA
  35. von Kármán self-preservation hypothesis for magnetohydrodynamic turbulence and its consequences for universality
  36. POWER ANISOTROPY IN THE MAGNETIC FIELD POWER SPECTRAL TENSOR OF SOLAR WIND TURBULENCE
  37. INVESTIGATION OF INTERMITTENCY IN MAGNETOHYDRODYNAMICS AND SOLAR WIND TURBULENCE: SCALE-DEPENDENT KURTOSIS
  38. DIRECTIONAL ALIGNMENT AND NON-GAUSSIAN STATISTICS IN SOLAR WIND TURBULENCE
  39. Transport of solar wind fluctuations: A two-component model
  40. Nonlocality and the critical Reynolds numbers of the minimum state magnetohydrodynamic turbulence
  41. On the accuracy of simulations of turbulence
  42. The third-order law for magnetohydrodynamic turbulence with shear: Numerical investigation
  43. The third-order law for magnetohydrodynamic turbulence with constant shear
  44. Statistical properties of solar wind discontinuities, intermittent turbulence, and rapid emergence of non-Gaussian distributions
  45. Solar Wind Turbulent Heating by Interstellar Pickup Protons: 2-Component Model
  46. Heating of the solar wind with electron and proton effects
  47. A Two-component Transport Model for Solar Wind Fluctuations: Waves plus Quasi-2D Turbulence
  48. A TURBULENCE-DRIVEN MODEL FOR HEATING AND ACCELERATION OF THE FAST WIND IN CORONAL HOLES
  49. The third-order law for increments in magnetohydrodynamic turbulence with constant shear
  50. Electron and proton heating by solar wind turbulence
  51. Generation of non-Gaussian statistics and coherent structures in ideal magnetohydrodynamics
  52. Anisotropic magnetohydrodynamic spectral transfer in the diffusion approximation
  53. Anisotropic Scaling of Magnetohydrodynamic Turbulence
  54. Turbulence transport throughout the heliosphere
  55. The impact of small-scale turbulence on laminar magnetic reconnection
  56. A two-component phenomenology for homogeneous magnetohydrodynamic turbulence
  57. Propagation and dissipation of Alfvén waves in stellar atmospheres permeated by isothermal winds
  58. Spacecraft observations of solar wind turbulence: an overview
  59. Direct comparisons of compressible magnetohydrodynamics and reduced magnetohydrodynamics turbulence
  60. Radial evolution of cross helicity in high-latitude solar wind
  61. Transport of cross helicity and radial evolution of Alfvénicity in the solar wind
  62. Reduced magnetohydrodynamics and parallel spectral transfer
  63. Impact of Hall effect on energy decay in magnetohydrodynamic turbulence
  64. Coronal Heating Distribution Due to Low‐Frequency, Wave‐driven Turbulence
  65. What can we infer about the underlying physics from burst distributions observed in an RMHD simulation?
  66. Heating of the low-latitude solar wind by dissipation of turbulent magnetic fluctuations
  67. Conditions for sustainment of magnetohydrodynamic turbulence driven by Alfvén waves
  68. A Reduced Magnetohydrodynamic Model of Coronal Heating in Open Magnetic Regions Driven by Reflected Low‐Frequency Alfven Waves
  69. Complexity in astroplasmas
  70. Kinetic helicity and MHD turbulence
  71. MHD‐driven Kinetic Dissipation in the Solar Wind and Corona
  72. Coronal Heating by Magnetohydrodynamic Turbulence Driven by Reflected Low-Frequency Waves
  73. Turbulence, Spatial Transport, and Heating of the Solar Wind
  74. Scaling of spectral anisotropy with magnetic field strength in decaying magnetohydrodynamic turbulence
  75. Scaling of Anisotropy in Hydromagnetic Turbulence
  76. Dynamical age of solar wind turbulence in the outer heliosphere
  77. Energy dynamics in linear MHD with ion parallel viscosity
  78. General second-rank correlation tensors for homogeneous magnetohydrodynamic turbulence
  79. Anisotropic three-dimensional MHD turbulence
  80. Phenomenology for the decay of energy‐containing eddies in homogeneous MHD turbulence
  81. Magnetic helicity in magnetohydrodynamic turbulence with a mean magnetic field
  82. Linear transport of solar wind fluctuations
  83. Reply [to “Comment on ‘Evolution of energy-containing turbulent eddies in the solar wind’ by W. H. Matthaeus, S. Oughton, D. H. Pontius Jr., and Y. Zhou”]
  84. The influence of a mean magnetic field on three-dimensional magnetohydrodynamic turbulence
  85. Transport theory and the WKB approximation for interplanetary MHD fluctuations
  86. Evolution of energy-containing turbulent eddies in the solar wind
  87. Relaxation in two dimensions and the ‘‘sinh‐Poisson’’ equation
  88. Properties of mass-loading shocks, 2. Magnetohydrodynamics
  89. Mass-loading and parallel magnetized shocks
  90. Decaying, two-dimensional, Navier-Stokes turbulence at very long times
  91. Selective decay and coherent vortices in two-dimensional incompressible turbulence
  92. Properties of mass-loading shocks: 1. Hydrodynamic considerations