Solar Coronal Heating and Limb Effect
Yi-Jia Zheng
TL;DR
This paper provides a quantitative explanation for the quiet solar coronal heating problem and the observed center-to-limb wavelength variations of solar lines, known as the limb effect.
Contribution
It offers a novel quantitative model that simultaneously explains coronal heating and limb effect phenomena in the Sun.
Findings
Quantitative calculations successfully explain coronal heating.
Model accounts for center-to-limb wavelength variations.
Results align with observational data.
Abstract
The quiet solar coronal heating problem and the observed center-to-limb wavelength variations of the solar lines (limb effect) can be explained. In this paper the quantitative calculations for these two phenomena are presented.
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Adaptive optics and wavefront sensing