{
  "abstract": "Building on recent advances in coronal spectropolarimetry, seismology, and magnetic-field inferences of Z. Yang et al. (2024) and A. R. Paraschiv (2026), we present the first application of the CLEDB IQUD inversion methodology to Mauna Loa Solar Observatory CoMP and UCoMP observations. Using spectropolarimetric IQU measurements together with coronal seismology-derived magnetic field B POS constraints, we recover vector magnetic field solutions across the off-limb solar corona accessible to the observations, demonstrating the feasibility of routine large-scale coronal vector magnetometry without the need for Stokes V observations.",
  "abstract_shown": true,
  "affiliations": [
    "National Solar Observatory",
    "High Altitude Observatory",
    "Southwest Research Institute"
  ],
  "article_type": null,
  "arxiv": null,
  "author_total": 4,
  "authors": [
    {
      "affs": [
        0
      ],
      "name": "Alin Razvan Paraschiv",
      "orcid": "0000-0002-3491-1983"
    },
    {
      "affs": [
        1
      ],
      "name": "Zihao Yang",
      "orcid": "0000-0002-4973-0018"
    },
    {
      "affs": [
        1
      ],
      "name": "Daniela Adriana Lacatus",
      "orcid": "0000-0003-2123-6605"
    },
    {
      "affs": [
        2
      ],
      "name": "Momchil Molnar",
      "orcid": "0000-0003-0583-0516"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/a92pewfyfhs4q.bib",
  "cited_by": 0,
  "doi": "10.3847/2041-8213/aead9e",
  "fulltext_url": null,
  "id": "a92pewfyfhs4q",
  "issns": [
    "2041-8213",
    "2041-8205"
  ],
  "landing_url": "https://iopscience.iop.org/article/10.3847/2041-8213/aead9e",
  "language": null,
  "licence": "CC-BY-4.0",
  "licence_label": "CC BY 4.0",
  "licence_source": "article",
  "licence_url": "https://creativecommons.org/licenses/by/4.0/",
  "metadata_licence": null,
  "native_subjects": [
    [
      "feed-journal",
      "astronomy/general"
    ],
    [
      "openalex",
      "3103|Solar and Space Plasma Dynamics"
    ]
  ],
  "openalex": "W7214758720",
  "pdf_url": "https://iopscience.iop.org/article/10.3847/2041-8213/aead9e/pdf",
  "pmcid": null,
  "pmid": null,
  "published": "2026-10-28",
  "publisher": "American Astronomical Society",
  "ris": "https://research.draconitic.com/paper/a92pewfyfhs4q.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:17:17Z",
      "native_id": "10.3847/2041-8213/aead9e",
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      "url": "https://iopscience.iop.org/article/10.3847/2041-8213/aead9e"
    },
    {
      "first_seen": "2026-10-30T12:18:13Z",
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      "url": "https://iopscience.iop.org/article/10.3847/2041-8213/aead9e"
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  "subjects": [
    {
      "field": "astronomy",
      "origin": "openalex:3103|Solar and Space Plasma Dynamics",
      "subfield": "stellar"
    }
  ],
  "title": "A First Global Full-vector Coronal Magnetic Field Inference Using MLSO CoMP and UCoMP Observations",
  "title_text": "A First Global Full-vector Coronal Magnetic Field Inference Using MLSO CoMP and UCoMP Observations",
  "type": "peer-reviewed",
  "updated_at": "2026-10-30T12:18:13Z",
  "url": "https://research.draconitic.com/paper/a92pewfyfhs4q",
  "venue": "The Astrophysical Journal Letters",
  "versions": []
}