Using eclipse observations to test scintillation models |
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Authors: | D Georgobiani J R Kuhn J M Beckers |
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Institution: | (1) National Solar Observatory, 88349 Sunspot, NM, U.S.A.;(2) Abastumani Astrophysical Observatory, 2a Al.Kazbegi ave., Tbilisi, Georgian Republic |
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Abstract: | 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 measureable time dependence to solar scintillation during an eclipse. This effect was observed during an annular solar eclipse and quantitatively compared with a scintillation model.Operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under cooperative agreement with the National Science Foundation. |
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