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[[Tập tin:Venuspioneeruv.jpg|250px|giữa|Cloud structure in Venus' atmosphere, revealed by ultraviolet observations. The characteristic V-shape of the clouds is due to the higher wind speed around the equator.]]
[[Image:Venuspioneeruv.jpg|250px|giữa|Cloud structure in Venus' atmosphere, revealed by ultraviolet observations. The characteristic V-shape of the clouds is due to the higher wind speed around the equator.]]
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