File:Unknown Pleasures knit sweater & Shergold Masquerader of Bernard Sumner - Joy Division Exhibition, Manchester, 2010 (2010-05-19 13.17.00 by Man Alive!).jpg

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Description The Joy Division Exhibition to mark the 30th Anniversary of Ian Cutis’ passing at fac251, Manchester
Date
Source Joy Division Exhibition
Author Man Alive!
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" The Joy Division Exhibition to mark the 30th Anniversary of Ian Cutis’ passing at fac251, Manchester "
References
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  • Jen Christiansen (2015-02-18). "Pop Culture Pulsar: Origin Story of Joy Division’s Unknown Pleasures Album Cover [Video]". Scientific American.
    • Eric Klotz (2012-10-18). Data Visualization Reinterpreted: The Story of Joy Division's "Unknown Pleasures" Album Design (video). YouTube. "Former Factory Records graphic designer Peter Saville discusses the design + effect of Joy Division's iconic "Unknown Pleasures" album cover. This video is the first in a series on the new language of data and its impact on culture and business."
    • Simon Mitton , ed. (1977) Cambridge Encyclopaedia of Astronomy, Prentice-Hall of Canada, by Terwin Copplestone Publishing, p. 111 ISBN: 9780131127227.
      "​[p111] Successive pulses from the first pulsar discovered, CP 1919, are here superimposed vertically. The pulses occur every 1.337 seconds. They are caused by rapidly spinning neutron star. "
    • Walter Herdeg , ed. (1974) Graphis Diagrams: The Graphic Visualization of Abstract Data, Zürich: Graphis Press
      "​[page] Von einem Computer erzeugte illustration von achtzig aufeinanderfolgenden Pulsperioden des ersten Pulsars, der beobachtet wurde. Die Durchschnittsbreite der Pulse ist weniger als eine 50tausendstel-Sekunde. Das Diagramm wurde vom Arecibo Radio-Observatorium in Puerto Rico hergestellt. Aus Scientific American, 'The Nature of Pulsars,' von J. P. Ostriker (U.S.A.). "
    • Jeremiah P. Ostriker. "The Nature of Pulsars". Scientific American (January 1971): 48-60.
      "​[p53] EIGHTY SUCCESSIVE PERIODS of the first pulsar observed, CP1919 (Cambridge pulsar at 19 hours 19 minutes right ascension), are stacked on top of one another using the average period of 1.33730 seconds in this computer-generated illustration produced at the Arecibo Radio Observatory in Puerto Rico. Although the leading edges of the radio pulses occur within a few thousandths of a second of the predicted times, the shape of the pulses is quite irregular. Some of this irregularity in radio reception is caused by the effects of transmission through the interstellar medium. The average pulse width is less than 50 thousandths of a second. "
  • Harold D. Craft, Jr. (1970-09) Radio Observations of the Pulse Profiles and Dispersion Measures of Twelve Pulsars[1] (Ph.D. Thesis, embedded PDF), Frank Donald Drake (advisor), Cornell University

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This image was originally posted to Flickr by Man Alive! at https://flickr.com/photos/24365773@N03/4622050896. It was reviewed on 1 February 2022 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

1 February 2022

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current09:59, 1 February 2022Thumbnail for version as of 09:59, 1 February 20222,304 × 3,072 (2.9 MB)Clusternote (talk | contribs)Transferred from Flickr via #flickr2commons

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