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 cloudy plumes that then subside. This storm is a strong source of radio emissions, which are interpreted by Cassini scientists as electric events like lightning on Earth.[1]
See also
References
- ↑ "The Dragon Storm". nasa.gov. NASA. Retrieved 22 May 2017.
External links
- NASA Astronomy Picture of the Day: Saturn's Dragon Storm (25 February 2005)
- NASA article on Dragon Storm
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