Coronal heating problem solution by means of axion origin photons
V.D. Rusov, I.V. Sharph, V.P. Smolyar, M.V. Eingorn, M.E. Beglaryan

TL;DR
This paper proposes that axions, originating from dark matter in the Sun's core, could explain the solar corona's high temperature, linking dark matter and solar physics through axion-origin photons.
Contribution
It introduces a novel hypothesis connecting dark matter axions with solar corona heating, suggesting a unified explanation for two longstanding mysteries.
Findings
Axion-origin photons may modulate solar corona temperature.
Dark matter density variations could influence solar corona heating.
Proposes a new link between dark matter and solar phenomena.
Abstract
In this paper we advocate for the idea that two seemingly unrelated mysteries with almost 90 year history -- the nature of dark matter and the million-degree solar corona -- may be but two sides of the same coin -- the axions of dark matter born in the core of the Sun and photons of axion origin in the million-degree solar corona, whose modulations are controlled by the anticorrelated modulation of the asymmetric dark matter (ADM) density in the solar interior.
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