Developed a metjod aimed at characterizing spots in active stars. The paper: “The GAPS programme at TNG LII. Spot modeling of V1298 Tau using SpotCCF tool” of C. di Mario (INAF – OAPA) recently appeared on A&A
The Sun regularly exhibits magnetic phenomena, including sunspots and solar flares, which are not only visually appealing but also crucial for in-depth study and understanding. This is because these phenomena arise from large-scale interactions between the solar magnetic field and its plasma. Moreover, they provide valuable insights into the structure of the Sun and its atmosphere. Almost all other
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