Dragon Storm (astronomy)

From Wikipedia, the free encyclopedia

Dragon Storm
Dragon Storm

Dragon Storm (dubbed so in September 2004 because of its unusual shape) is a name given to a large, bright and complex convective storm in Saturn's southern hemisphere. The storm appears to be long-lived and periodically flares up to produce dramatic white plumes which then subside. The storm was a strong source of radio emissions. [1]

[edit] References

  1. ^ NASA NIX image search, image description[1]

[edit] See also