Image Details
Caption: Figure 5.
Spectroscopic analysis of the Fe I 6173.34 Å line in different solar features. Top panel: a partial raw spectral image, with the line position circled. Bottom panel: temporal variation of the line’s full width at half maximum (FWHM) in a sunspot umbra, a dark filament, and a quiet-Sun region, demonstrating magnetic and thermal broadening.
© 2026. The Author(s). Published by the American Astronomical Society.