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Shadow bands observed during the total solar eclipse of 4 December 2002, by high-resolution imaging
This paper presents results of a comparison between the characteristics of shadow bands recorded during the total solar eclipse of 4 December 2002 in Botswana, and the theory of Codona (Codona, 1986, Astronomy and Astrophysics 164, 415–427). For the first time the analysis was based on images of the...
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Published in: | Journal of atmospheric and solar-terrestrial physics 2005-07, Vol.67 (10), p.899-906 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | This paper presents results of a comparison between the characteristics of shadow bands recorded during the total solar eclipse of 4 December 2002 in Botswana, and the theory of Codona (Codona, 1986, Astronomy and Astrophysics 164, 415–427). For the first time the analysis was based on images of the phenomenon and not photometric data. Thanks to this, use was made of high spatial resolution and detailed plots of power spectra were obtained. The plots’ shapes are in excellent agreement with those predicted by theory. From them, the height of the scattering layer producing shadow bands was inferred. |
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ISSN: | 1364-6826 1879-1824 |
DOI: | 10.1016/j.jastp.2005.02.012 |