{
  "annotation_id": "318a8472-4bf6-4f7a-ada8-bdd74c4e3357",
  "date_created": "2026-03-02T18:00:36.036000Z",
  "date_modified": "2026-03-02T18:00:36.036000Z",
  "file_hash": "ab26ab185b78b9434e73d43f07d92cb64dae36148e324f69da0161e490d0d399",
  "private": false,
  "record": {
    "abstract": "Weak turbulence of magnetohydrodynamic (MHD) waves in strongly magnetized\nplasma is studied when the thermal pressure is less than the magnetic field\npressure. In this situation the main nonlinear mechanism is the resonance\nscattering of fast magneto-acoustic and Alfvenic waves on slow magneto-acoustic\nwaves. As a result, the former waves serve as the high-frequency waves with\nrespect to the latter ones so that the total number of HF waves - an adiabatic\ninvariant - conserves additionally. In the weak turbulence regime this\ninvariant is shown to generate the Kolmogorov type spectrum with a constant\nflux of HF waves towards large-scale region. In the short-wave region another\nKolmogorov spectrum can be realized with a constant energy flux. The explicit\nangle dependences for both types of turbulent spectra are found for the\npropagation angles close to the direction of a mean magnetic field.",
    "arxiv_id": "physics/0109066",
    "authors": [
      "Evgenii A. Kuznetsov"
    ],
    "categories": [
      "physics.plasm-ph",
      "physics.flu-dyn"
    ],
    "doi": "10.1134/1.1427116",
    "title": "Weak magnetohydrodynamic turbulence of magnetized plasma",
    "url": "https://arxiv.org/abs/physics/0109066"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "b856a6f1-41d6-4eb3-8d5e-d77565168330",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}