The Surface of the Nearest Star
Metadata
- Publisher
- SMPTE
- Doc Type
- Journal Article
- Article Type
- research-article
- Abstract
- Taking motion pictures of celestial phenomona that show change is not as simple as it would first appear. Work on spectroheliokinematography was started in 1928, and in 1931 the instrumentation was donated to the University of Michigan by the founders of the McMath-Hulbert Observatory. The combined tower telescope and spectroheliokinemalograph of this observatory. now one of the most powerful pieces of solar apparatus in the world, is described and some of the solar data obtained with it are discussed.
- Publication Date
- 1939-03-01
- DOI
10.5594/J12016- Link
- https://doi.org/10.5594/J12016
- Author(s)
- R. R. McMath
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R. R. McMath; The Surface of the Nearest Star, Journal of the Society of Motion Picture Engineers ( Volume: 32, Issue: 3, March 1939); SMPTE, 1939. Available at https://doi.org/10.5594/J12016
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R. R. McMath; The Surface of the Nearest Star, Journal of the Society of Motion Picture Engineers ( Volume: 32, Issue: 3, March 1939); SMPTE, 1939. Available at https://doi.org/10.5594/J12016
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R. R. McMath; The Surface of the Nearest Star, Journal of the Society of Motion Picture Engineers ( Volume: 32, Issue: 3, March 1939); SMPTE, 1939. Available at https://doi.org/10.5594/J12016
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<span class="citation">R. R. McMath; <cite>The Surface of the Nearest Star</cite>, Journal of the Society of Motion Picture Engineers ( Volume: 32, Issue: 3, March 1939); SMPTE, 1939. Available at <a href="https://doi.org/10.5594/J12016" target="_blank" rel="noopener">https://doi.org/10.5594/J12016</a></span>
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R. R. McMath; The Surface of the Nearest Star, Journal of the Society of Motion Picture Engineers ( Volume: 32, Issue: 3, March 1939); SMPTE, 1939
doi: 10.5594/J12016
url: https://doi.org/10.5594/J12016
doi: 10.5594/J12016
url: https://doi.org/10.5594/J12016
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<li> R. R. McMath; <cite id="bib-10-5594-j12016">The Surface of the Nearest Star</cite>, Journal of the Society of Motion Picture Engineers ( Volume: 32, Issue: 3, March 1939); SMPTE, 1939 <span class="doi">10.5594/J12016</span> </li>