{
  "abstract": "The large-scale structure of the Solar System is conventionally explained by gravitational orbital dynamics, whereas the interplanetary magnetic environment is explained by solar-origin plasma and magnetic-field processes. This study proposes the hypothesis that these two levels of organization may not be entirely independent and that frequency-selective electromagnetic coupling between the Sun and planets may contribute to central-motion organization.\n\nThe model predicts that not all common frequencies have the same physical significance. Instead, the highest significant frequency components within the relevant measurement band of interacting Sun-centered and planet-centered electromagnetic-plasma systems should preferentially approach or overlap.\n\nPublished Wind–ARTEMIS observations reported common low-frequency spectral peaks between upstream solar-wind/interplanetary magnetic-field measurements and magnetotail measurements near lunar-orbit distance, particularly at approximately 0.64–0.69 mHz and 0.89–0.93 mHz. In contrast, significant ARTEMIS peaks at approximately 0.37–0.47 mHz lacked corresponding Wind or ACE peaks.\n\nThese observations are reinterpreted as a test case for frequency-selective coupling. The proposed mechanism is not considered demonstrated; rather, the study develops falsifiable predictions involving cross-spectral coherence, phase relationships, spectral ordering, repeated lunar magnetotail passages, control intervals, and comparative observations at other planets.",
  "abstract_shown": true,
  "affiliations": [
    "independent researcher"
  ],
  "article_type": null,
  "arxiv": null,
  "author_total": 1,
  "authors": [
    {
      "affs": [
        0
      ],
      "name": "Kadir Gürel",
      "orcid": "0009-0004-0475-4608"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/d47thmqvdvedq.bib",
  "cited_by": 0,
  "doi": "10.5281/zenodo.23661364",
  "fulltext_url": null,
  "id": "d47thmqvdvedq",
  "issns": [],
  "landing_url": "https://zenodo.org/records/23661364",
  "language": "eng",
  "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": [],
  "openalex": null,
  "pdf_url": null,
  "pmcid": null,
  "pmid": null,
  "published": "2026-10-26",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/d47thmqvdvedq.ris",
  "sources": [
    {
      "first_seen": "2026-11-09T12:21:00Z",
      "native_id": "23661364",
      "source": "zenodo",
      "url": "https://zenodo.org/records/23661364"
    }
  ],
  "subjects": [],
  "title": "A Testable Hypothesis of Frequency-Selective Electromagnetic Coupling in Sun–Planet Systems: Reinterpreting Wind–ARTEMIS Low-Frequency Spectral Overlaps",
  "title_text": "A Testable Hypothesis of Frequency-Selective Electromagnetic Coupling in Sun–Planet Systems: Reinterpreting Wind–ARTEMIS Low-Frequency Spectral Overlaps",
  "type": "preprint",
  "updated_at": "2026-11-09T12:21:00Z",
  "url": "https://research.draconitic.com/paper/d47thmqvdvedq",
  "venue": "Zenodo",
  "versions": []
}