Dragon Storm (astronomy)

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Dragon Storm

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. The Saturnian storm appears to be long-lived and periodically flares up to produce dramatic white plumes which then subside. The storm is a strong source of radio emissions.[1]

[edit] See also

[edit] References

  1. ^ "Saturn's Dragon Storm". http://www.thunderbolts.info/tpod/2006/arch06/060714dragonstorm.htm. Retrieved 8 July 2011. 

[edit] External links
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