Dragon Storm (astronomy)

The Dragon Storm is a giant thunderstorm located in Saturn's Southern hemisphere, which is labeled as the "storm alley" region. The storm could have a range of 2,000 miles (3,200 km) or more, and can be compared to the electric thunderstorms of Earth. It acquires its energy in the deep layers of Saturn's atmosphere and produces radio waves that reflect during its burst of short static which helped Cassini detect it.

The Dragon Storm (named in September 2004 for 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 is similar to the extreme conditions on Jupiter at the site of its Great Red Spot, an anticyclonic storm that has been continually observed since 1830. The Dragon Storm is a strong source of radio emissions, which are interpreted by Cassini scientists as electric events similar to lightning on Earth.^[1]

Cassini detected a burst of radio emissions when the Dragon Storm started rising over the horizon during the night time of the planet. The burst came to a stop when it hit the sunlight. During the night time of Saturn, the storm starts; as soon as it hits sunlight, it completely stops. This pattern repeats, seeming to go on and off for a few weeks as Saturn rotates.

See also

• Extraterrestrial cyclone
• Great Dark Spot
• Great White Spot
• Oval BA
• Small Dark Spot

References

External links

• NASA Astronomy Picture of the Day: Saturn's Dragon Storm (25 February 2005)
• Fischer, Georg; Gurnett, Donald A.; Kurth, William S.; Akalin, Ferzan; Zarka, Philippe; Dyudina, Ulyana A.; Farrell, William M.; Kaiser, Michael L. (2008). "Atmospheric Electricity at Saturn". Space Science Reviews. 137 (1–4): 271–285. Bibcode:2008SSRv..137..271F. doi:10.1007/s11214-008-9370-z.

This page was last edited on 16 March 2024, at 08:36