Solar Coronal Heating and Wind Acceleration from Fractal Vacuum Geometry

Zenodo (CERN European Organization for Nuclear Research) 2026 Open access

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Authors: Edgar Marquez Escalante
DOI: 10.5281/zenodo.18777560
Cited by: 0

Abstract

CORONA.pdf: Solar coronal heating via topological phase transition (amplification 25.8×, Fe enrichment 3.5×, He depletion 0.5×). Error

Fields of Study & Subjects

Solar and Space Plasma Dynamics Stellar planetary and galactic studies Advanced Mathematical Theories and Applications

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
25 February 2026
Language
EN