Why every observatory needs a disco ball
Physics Education, vol. 59, pp. 025012
Abstract
Abstract Commercial disco balls provide a safe, effective and instructive way of observing the Sun. We explore the optics of solar projections with disco balls, and find that while sunspot observations are challenging, the solar disk and its changes during eclipses are easy and fun to observe. We explore the disco ball’s potential for observing the moon and other bright astronomical phenomena.
Authors 8
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Robert Cumming corresponding
Chalmers University of Technology
Affiliation as printed
Onsala Space Observatory, Department of Space, Earth and Environment, Chalmers University of Technology, Onsala, SE-439 92, Sweden
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Leibniz Institute for Astrophysics Potsdam
Affiliation as printed
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
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Livia Pietrow Aachen
Affiliation as printed
Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands
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Affiliation as printed
Department of Astronomy, Stockholm University, 106 91 Stockholm, Sweden
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Affiliation as printed
Observatoire de l’Université de Genève, Chemin Pegasi 51, 1290 Versoix, Switzerland
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Casper Pietrow Aachen
Affiliation as printed
Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands
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Centre National de la Recherche Scientifique · Université Toulouse III - Paul Sabatier · Institut de Recherche en Astrophysique et Planétologie
Affiliation as printed
Institut de Recherche en Astrophysique et Planétologie (IRAP), Université Toulouse III—Paul Sabatier, CNRS, CNES, 9 Av. du colonel Roche, 31028 Toulouse Cedex 04, France
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Affiliation as printed
Institute for Solar Physics, Department of Astronomy, Stockholm University, Roslagstullsbacken 21, Stockholm, Sweden
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References 22
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