Abstract:ABSTRACT. Stellar scintillation has been measured from 0.9 to 1.7 mm over a wide range of elevation angles. The pupil from a 3.5 m telescope was imaged onto a mask with four circular apertures of scaled diameters 0.1, 0.2, 0.75, and 1.5 m, which were, in turn, reimaged onto InGaAs photodiodes digitally sampled at 10 kHz. The entire 3.5 m pupil was also imaged onto a fifth photodiode. Since all five fluxes were recorded simultaneously, the influence of aperture diameter on scintillation statistics can be readil… Show more
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