Shadow bands observed during the total solar eclipse of 4 December 2002, by high-resolution imaging

Details Shadow bands observed during the total solar eclipse of 4 December 2002, by high-resolution imaging Shadow bands observed during the total solar eclipse of 4 December 2002, by high-resolution imaging

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005jastp..67..899g&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 67, Issue 10, p. 899-906.

Physics

Scientific paper

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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