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Dragon Storm (astronomy)
Dragon Storm (dubbed so in September 2004 because of its unusual shape) is a large, bright and complex convective storm in Saturn's southern hemisphere. It appears to be long-lived and periodically flares up to produce dramatic white plumes that then subside. The storm is a strong source of radio emissions.
== See also ==
*Extraterrestrial cyclone
*Great Red Spot
*Oval BA
*Great Dark Spot
*Small Dark Spot
抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』
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