Using eclipse observations to test scintillation models

Details Using eclipse observations to test scintillation models Using eclipse observations to test scintillation models

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..156....1g&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 156, no. 1, p. 1-5

Physics

2

Luminous Intensity, Scintillation, Solar Eclipses, Solar Physics, Sun, Brightness, Mathematical Models, Power Spectra, Solar Atmosphere, Variations

Scientific paper

Near second and third contact during a solar eclipse the spatial spectrum of the solar illumination changes as the relative power at high spatial frequencies increases strongly. Since groundlevel atmospheric scintillation depends on a weighted integral of the image power spectrum, we can expect to see a measurable time dependence to solar scintillation during an eclipse. This effect was observed during an annular solar eclipse and quantitatively compared with a scintillation model.

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