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RickStudent, Philosopher, Writer, Developer
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The Great Hall at the University of Leeds
Photo Credit: By Betty Longbottom, CC BY-SA 2.0, https://commons.wikimedia.org/w/index.php?curid=10496396
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logo for University of Leeds
Photo Credit: By University of Leeds Image Guidelines, Fair use, https://en.wikipedia.org/w/index.php?curid=57420134
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Bragg X-ray Spectrometer
Photo Credit: https://commons.wikimedia.org/w/index.php?curid=36214143
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University of Adelaide, Barr Smith Lawns
Photo Credit: By Pdfpdf (talk) - My camera, my software and I created this work entirely by ourselves., Public Domain, https://commons.wikimedia.org/w/index.php?curid=18049023
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logo for University of Adelaide
Photo Credit: By Obtained from https://www.adelaide.edu.au and copyright owned by the University of Adelaide., Fair use, https://en.wikipedia.org/w/index.php?curid=56077618
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William Henry Bragg — c 1915
Photo Credit: By Nobel foundation - Public Domain, https://commons.wikimedia.org/w/index.php?curid=33407292
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Bohr and Margrethe Nørlund on their engagement in 1910
Photo Credit: Niels Bohr Institute, Public Domain, https://commons.wikimedia.org/w/index.php?curid=24652845
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Margrethe Nørlund Bohr
Photo Credit: Public Domain, https://commons.wikimedia.org/w/index.php?curid=24652845
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Bohr model - hydrogen atom — The cake model of the hydrogen atom (Z = 1) or a hydrogen-like ion (Z > 1), where the negatively charged electron confined to an atomic shell encircles a small, positively charged atomic nucleus and where an electron jumps between orbits, is accompanied by an emitted or absorbed amount of electromagnetic energy (hν). The orbits in which the electron may travel are shown as grey circles; their radius increases as n2, where n is the principal quantum number. The 3 → 2 transition depicted here produces the first line of the Balmer series, and for hydrogen (Z = 1) it results in a photon of wavelength 656 nm (red light).
Photo Credit: By JabberWok, CC BY-SA 3.0, https://commons.wikimedia.org/w/index.php?curid=2639910
Bohr model - hydrogen atom The cake model of the hydrogen atom (Z = 1) or a hydrogen-like ion (Z > 1), where the negatively charged electron confined to an atomic shell encircles a small, positively charged atomic nucleus and where an electron jumps between orbits, is accompanied by an emitted or absorbed amount of electromagnetic energy (hν). The orbits in which the electron may travel are shown as grey circles; their radius increases as n2, where n is the principal quantum number. The 3 → 2 transition depicted here produces the first line of the Balmer series, and for hydrogen (Z = 1) it results in a photon of wavelength 656 nm (red light).
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Werner Heisenberg (left) with Bohr at the Copenhagen Conference in 1934
Photo Credit: By Fermilab, U.S. Department of Energy - Public Domain, https://commons.wikimedia.org/w/index.php?curid=6877522
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Niels Bohr, physicist
Photo Credit: Niels Bohr's Nobel Prize biography, from 1922, Public Domain, https://commons.wikimedia.org/w/index.php?curid=288274