“…Despite that initial interest, the OAUC would not leap into this new field, remaining committed to its astronomical ephemerides' calculation program and the teaching of practical astronomy and celestial mechanics. Only in the 1920s would an astrophysics program related to the study of the Sun be implemented at OAUC (Bonifácio, 2017). In 1926, Francisco Costa Lobo (1864–1945), then director of OAUC, installed a systematic daily solar observations program of sunspots, faculae, filaments, and prominences, on Ca II and Hα lines.…”