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Seventy-Four Minutes of Observation, but What Gain for Science?

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Part of the book series: Astronomers' Universe ((ASTRONOM))

Abstract

It’s all very well setting up a record observation time, but that wasn’t really the main objective for the scientists who set off on this adventure. One might say that it was only a secondary result. It was the Sun and its corona that really interested us. So what discoveries were made thanks to the three exceptional circumstances we benefited from: the long period of totality, the slow scan of the chromosphere just before and just after totality, and the excellent access to infrared emissions from such a high flight path?

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Notes

  1. 1.

    P. Lamy et al.: No evidence of a circumsolar dust ring from the infrared observations of the 1991 solar eclipse. In: Science 257, 1377 (1992).

  2. 2.

    L.I. Shestakova et al.: The velocity of the dust near the Sun during the solar eclipse of March 29, 2006 and sun-grazing comets. In: 2010arXiv1003.2818S (2010).

  3. 3.

    Infrared Astronomical Satellite (IRAS), launched by NASA on 25 January 1983.

  4. 4.

    L.I. Shestakova: The beta Pictoris phenomenon near the Sun. In: Astronomical and Astrophysical Transactions 22 (2), 191–211 (2003), 10.1080/1055679031000080339

  5. 5.

    http://www.forum-ovni-ufologie.com/t8611-la-guerre-des-mondes-les-martiens-d-orson-welles-le-30-octobre-1938#ixzz2a3iZLX5O

  6. 6.

    https://en.wikipedia.org/wiki/Unidentified_flying_object

  7. 7.

    https://www.cnes-geipan.fr

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Léna, P. (2015). Seventy-Four Minutes of Observation, but What Gain for Science?. In: Racing the Moon’s Shadow with Concorde 001. Astronomers' Universe. Springer, Cham. https://doi.org/10.1007/978-3-319-21729-1_6

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