Work

Wave Physics-Based Explanation of the Anomalous Heating of Stellar Coronae.v2

Year: 2025

Type: article

Abstract: We present a compact, testable coronal-heating framework in which MHD waves experiencepartial reflection at steep stratification (the transition region, TR), naturally seeding counter-propagating content that dissipates via phase mixing and resonant absorption. Unlike opticsanalogies, energy reflection and transmission are derived from linear MHD with proper boundaryconditions: (i) an energy-impedance formulation for sharp interfaces, (ii) WKB transmission ingraded layers, and (iii) an oblique-incidence, mode-coupling recipe (Appendix A). A closedheating relation

Source: Zenodo (CERN European Organization for Nuclear Research)

DOI: 10.5281/zenodo.17080216

Author: neşet erol, uğur

Language: English

Topic: Solar and Space Plasma Dynamics

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: green

OpenAlex ID: W7080599625

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