Image Details
Caption: Figure 10.
Comparison of the Ca IIλ8542 line between the templates and the observed solar spectrum at solar parameters. The shaded region and the inset indicate the 1 Å line-core window. The spectral resolving power is ≥300, 000, and solar rotational broadening (﹩v\sin i=1.6\,{\rm{km}}\,{{\rm{s}}}^{-1}﹩) is included.
© 2026. The Author(s). Published by the American Astronomical Society.