All Stories

  1. Evolution of similarity lengths in anisotropic magnetohydrodynamic turbulence
  2. Reduced MHD in Astrophysical Applications: Two-dimensional or Three-dimensional?
  3. A GENERALIZED TWO-COMPONENT MODEL OF SOLAR WIND TURBULENCE AND AB INITIO DIFFUSION MEAN-FREE PATHS AND DRIFT LENGTHSCALES OF COSMIC RAYS
  4. VARIANCE ANISOTROPY IN KINETIC PLASMAS
  5. Variance anisotropy in compressible 3-D MHD
  6. Intermittency, nonlinear dynamics and dissipation in the solar wind and astrophysical plasmas
  7. Anisotropy in solar wind plasma turbulence
  8. DISSIPATION AND RECONNECTION IN BOUNDARY-DRIVEN REDUCED MAGNETOHYDRODYNAMICS
  9. NONLINEAR AND LINEAR TIMESCALES NEAR KINETIC SCALES IN SOLAR WIND TURBULENCE
  10. COMPLEXITY AND DIFFUSION OF MAGNETIC FLUX SURFACES IN ANISOTROPIC TURBULENCE
  11. MAGNETIC FIELD LINE RANDOM WALK IN MODELS AND SIMULATIONS OF REDUCED MAGNETOHYDRODYNAMIC TURBULENCE
  12. ON THE ORIGIN OF ANISOTROPY IN MAGNETOHYDRODYNAMIC TURBULENCE: THE ROLE OF HIGHER-ORDER CORRELATIONS
  13. Generation of X-points and secondary islands in 2D magnetohydrodynamic turbulence
  14. Solar wind fluctuations and the von Kármán–Howarth equations: The role of fourth-order correlations
  15. Scaling anisotropy of the power in parallel and perpendicular components of the solar wind magnetic field
  16. LOCAL ANISOTROPY, HIGHER ORDER STATISTICS, AND TURBULENCE SPECTRA
  17. von Kármán self-preservation hypothesis for magnetohydrodynamic turbulence and its consequences for universality
  18. POWER ANISOTROPY IN THE MAGNETIC FIELD POWER SPECTRAL TENSOR OF SOLAR WIND TURBULENCE
  19. INVESTIGATION OF INTERMITTENCY IN MAGNETOHYDRODYNAMICS AND SOLAR WIND TURBULENCE: SCALE-DEPENDENT KURTOSIS
  20. DIRECTIONAL ALIGNMENT AND NON-GAUSSIAN STATISTICS IN SOLAR WIND TURBULENCE
  21. Transport of solar wind fluctuations: A two-component model
  22. Nonlocality and the critical Reynolds numbers of the minimum state magnetohydrodynamic turbulence
  23. On the accuracy of simulations of turbulence
  24. The third-order law for magnetohydrodynamic turbulence with shear: Numerical investigation
  25. The third-order law for magnetohydrodynamic turbulence with constant shear
  26. Statistical properties of solar wind discontinuities, intermittent turbulence, and rapid emergence of non-Gaussian distributions
  27. Solar Wind Turbulent Heating by Interstellar Pickup Protons: 2-Component Model
  28. Heating of the solar wind with electron and proton effects
  29. A Two-component Transport Model for Solar Wind Fluctuations: Waves plus Quasi-2D Turbulence
  30. A TURBULENCE-DRIVEN MODEL FOR HEATING AND ACCELERATION OF THE FAST WIND IN CORONAL HOLES
  31. The third-order law for increments in magnetohydrodynamic turbulence with constant shear
  32. Electron and proton heating by solar wind turbulence
  33. Generation of non-Gaussian statistics and coherent structures in ideal magnetohydrodynamics
  34. Anisotropic magnetohydrodynamic spectral transfer in the diffusion approximation
  35. Anisotropic Scaling of Magnetohydrodynamic Turbulence
  36. Turbulence transport throughout the heliosphere
  37. The impact of small-scale turbulence on laminar magnetic reconnection
  38. A two-component phenomenology for homogeneous magnetohydrodynamic turbulence
  39. Propagation and dissipation of Alfvén waves in stellar atmospheres permeated by isothermal winds
  40. Spacecraft observations of solar wind turbulence: an overview
  41. Direct comparisons of compressible magnetohydrodynamics and reduced magnetohydrodynamics turbulence
  42. Radial evolution of cross helicity in high-latitude solar wind
  43. Transport of cross helicity and radial evolution of Alfvénicity in the solar wind
  44. Reduced magnetohydrodynamics and parallel spectral transfer
  45. Impact of Hall effect on energy decay in magnetohydrodynamic turbulence
  46. Coronal Heating Distribution Due to Low‐Frequency, Wave‐driven Turbulence
  47. What can we infer about the underlying physics from burst distributions observed in an RMHD simulation?
  48. Heating of the low-latitude solar wind by dissipation of turbulent magnetic fluctuations
  49. Conditions for sustainment of magnetohydrodynamic turbulence driven by Alfvén waves
  50. A Reduced Magnetohydrodynamic Model of Coronal Heating in Open Magnetic Regions Driven by Reflected Low‐Frequency Alfven Waves
  51. Complexity in astroplasmas
  52. Kinetic helicity and MHD turbulence
  53. MHD‐driven Kinetic Dissipation in the Solar Wind and Corona
  54. Coronal Heating by Magnetohydrodynamic Turbulence Driven by Reflected Low-Frequency Waves
  55. Turbulence, Spatial Transport, and Heating of the Solar Wind
  56. Scaling of spectral anisotropy with magnetic field strength in decaying magnetohydrodynamic turbulence
  57. Scaling of Anisotropy in Hydromagnetic Turbulence
  58. Dynamical age of solar wind turbulence in the outer heliosphere
  59. Energy dynamics in linear MHD with ion parallel viscosity
  60. General second-rank correlation tensors for homogeneous magnetohydrodynamic turbulence
  61. Anisotropic three-dimensional MHD turbulence
  62. Phenomenology for the decay of energy‐containing eddies in homogeneous MHD turbulence
  63. Magnetic helicity in magnetohydrodynamic turbulence with a mean magnetic field
  64. Linear transport of solar wind fluctuations
  65. 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”]
  66. The influence of a mean magnetic field on three-dimensional magnetohydrodynamic turbulence
  67. Transport theory and the WKB approximation for interplanetary MHD fluctuations
  68. Evolution of energy-containing turbulent eddies in the solar wind
  69. Relaxation in two dimensions and the ‘‘sinh‐Poisson’’ equation
  70. Properties of mass-loading shocks, 2. Magnetohydrodynamics
  71. Mass-loading and parallel magnetized shocks
  72. Decaying, two-dimensional, Navier-Stokes turbulence at very long times
  73. Selective decay and coherent vortices in two-dimensional incompressible turbulence
  74. Properties of mass-loading shocks: 1. Hydrodynamic considerations