All Stories

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