2017
DOI: 10.4000/cahierscfv.773
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Costa Lobo (1864-1945), the Coimbra Spectroheliograph and the Internationalisation of Portuguese Astronomy

Abstract: At the beginning of the 20th century, Portuguese astronomy was still firmly anchored in the past. Only astronometric research was pursued and Portuguese professional astronomers seldom published their results. This situation changed in the 1910s thanks to the actions of Francisco Miranda da Costa Lobo (1864Lobo ( -1945. Costa Lobo initiated the construction in Coimbra of a world-class solar observing facility in close co-operation with observatory astronomers based in Meudon. Recognising the importance of inte… Show more

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“…From 1926 until 1944, the astronomical observatory made daily observations of sunspots, faculae, filaments, and prominences on lines Ca II and Hα using a spectroheliograph installed primarily in the IGUC premises (Figure 5). These observations were published in catalogues (Bonifácio, 2017). In the 1950s, that equipment was relocated to the Santa Clara campus.…”
Section: The Solar Images Collectionmentioning
confidence: 99%
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“…From 1926 until 1944, the astronomical observatory made daily observations of sunspots, faculae, filaments, and prominences on lines Ca II and Hα using a spectroheliograph installed primarily in the IGUC premises (Figure 5). These observations were published in catalogues (Bonifácio, 2017). In the 1950s, that equipment was relocated to the Santa Clara campus.…”
Section: The Solar Images Collectionmentioning
confidence: 99%
“…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.…”
Section: A Brief History Of Ogauc and Its Former Observatoriesmentioning
confidence: 99%