{
  "abstract": "We performed three-dimensional radiative magnetohydrodynamic(3D RMHD) simulations in an upward-directed (positive-polarity) open magnetic field with an initial background strength of 10 G. We identified vortex-associated spicule-like events and carried out a detailed analysis of one representative event. Prior to the formation of this spicule-like event, a photospheric vortex appears and twists the magnetic field lines, then develops upward into higher atmospheric layers, forming a magnetic tornado system. This event is generated during this process. At the periphery of this magnetic tornado, twisted magnetic field lines with negative vertical components reconnect with both external positive-polarity background fields and central positive-polarity fields. The magnetic reconnection sites rise and rotate together with the developed magnetic tornado, and many jet-like substructures in this event are closely associated with plasma upward ejections from these reconnection regions. A vertical force analysis shows that, for this event, plasma uplift in the photosphere and lower chromosphere is dominated by the pressure-gradient force, whereas in the upper chromosphere, the Lorentz force gradually becomes dominant. At a height of about 4 Mm above the solar surface, this event produces a mean upward mass flux density on the order of $10^{-7}~{\\rm kg~m^{-2}~s^{-1}}$ and a mean upward Poynting flux density of approximately $525~{\\rm W~m^{-2}}$. The wave-mode decomposition results show that the energy transport associated with the rotational spicule-like event is dominated by the Alfvén mode. Alfvén waves, fast-mode waves, and slow-mode waves carry energy into the lower corona in an approximate ratio of $10:7:3$.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2610.13173",
  "author_total": 6,
  "authors": [
    {
      "name": "Liufan Gong"
    },
    {
      "name": "Lei Ni"
    },
    {
      "name": "Guanchong Cheng"
    },
    {
      "name": "Jiajia Liu"
    },
    {
      "name": "Quan Xie"
    },
    {
      "name": "Robert Erdélyi"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/0mmfacryk7h21.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2610.13173",
  "fulltext_url": null,
  "id": "0mmfacryk7h21",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2610.13173",
  "language": null,
  "licence": "LicenseRef-arXiv-nonexclusive-1.0",
  "licence_label": "arXiv licence",
  "licence_source": "article",
  "licence_url": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
  "metadata_licence": "CC0-1.0",
  "native_subjects": [
    [
      "arxiv",
      "astro-ph.SR"
    ]
  ],
  "openalex": null,
  "pdf_url": "https://arxiv.org/pdf/2610.13173",
  "pmcid": null,
  "pmid": null,
  "published": "2026-10-09",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/0mmfacryk7h21.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:28:36Z",
      "native_id": "2610.13173",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2610.13173"
    }
  ],
  "subjects": [
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.SR",
      "subfield": "stellar"
    }
  ],
  "title": "Formation Dynamics of a Rotating Solar Spicule-like Event and Associated Energy-Mass Transport",
  "title_text": "Formation Dynamics of a Rotating Solar Spicule-like Event and Associated Energy-Mass Transport",
  "type": "preprint",
  "updated_at": "2026-10-30T12:28:36Z",
  "url": "https://research.draconitic.com/paper/0mmfacryk7h21",
  "venue": "arXiv",
  "versions": []
}