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Fig. 1


Images showing the six recordings of three Jovian bolides. Differences in sizes are caused by differences in the original data and depend on the specifics of the telescope and camera used. The central column corresponds to the brightest frame where each impact is visible (circles). The left and right columns correspond to frames recorded one second before and after the impact brightest frame. The impact is still barely visible in the right column for the A.W. and G.H. recordings obtained with the largest aperture telescopes.

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