[HTML][HTML] Solar Hα excess during Solar Cycle 24 from full-disk filtergrams of the Chromospheric Telescope

A Diercke, C Kuckein, PW Cauley… - Astronomy & …, 2022 - aanda.org
Context. The chromospheric Hα spectral line is a strong line in the spectrum of the Sun and
other stars. In the stellar regime, this spectral line is already used as a powerful tracer of …

Characterization of chromospheric activity based on Sun‐as‐a‐star spectral and disk‐resolved activity indices

E Dineva, J Pearson, I Ilyin, M Verma… - Astronomische …, 2022 - Wiley Online Library
The strong chromospheric absorption lines Ca ii H & K are tightly connected to stellar
surface magnetic fields. Only for the Sun, spectral activity indices can be related to evolving …

Application of Curl of the Counter Tangential Vector Field for Edge Detection of Color Images

S Wiangsamut, N Eua-Anant… - วารสาร วิชาการ …, 2022 - ph01.tci-thaijo.org
Abstract Information regarding edges is essential for many fields of image processing. A
classical edge detection method, such as the Canny algorithm, uses the gradient of an …