All Stories

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