Huge sun tornado discovered

Scientists at Aberystwyth University have discovered solar tornadoes several times as wide as the Earth on the face of the sun.

Dr Xing Li and Dr Huw Morgan from the Institute of Mathematics and Physics are presenting a movie of one of the tornadoes at the National Astronomy Meeting 2012 in Manchester today, Thursday 29th March 2012.

The solar tornado was discovered using the Atmospheric Imaging Assembly (AIA) telescope on board the Solar Dynamic Observatory (SDO) satellite.

“This is perhaps the first time that such a huge solar tornado is filmed by an imager. Previously much smaller solar tornadoes were found by SOHO satellite, but they were not filmed,” says Dr. Xing Li, of Aberystwyth University.
 
Dr. Huw Morgan, co-discover of the solar tornado, adds, “This unique and spectacular tornado must play a role in triggering global solar storms.”
 
The AIA saw superheated gases as hot as 50 000 – 2 000 000 Kelvin sucked from the root of a dense structure called prominence, and spiral up into the high atmosphere and travel about 200 000 kilometres along helical paths for a period of at least three hours.  The tornadoes were observed on 25 September 2011.
 
The hot gases in the tornadoes have speeds as high as 300,000 km per hour. Gas speeds of terrestrial tornadoes can reach 150km per hour.
 
The tornadoes often occur at the root of huge coronal mass ejections. When heading toward the Earth, these coronal mass ejections can cause significant damage to the Earth’s space environment, satellites, even knock out the electricity grid.
 
The solar tornadoes drag winding magnetic field and electric currents into the high atmosphere.  It is possible that the magnetic field and currents play a key role in driving the coronal mass ejections.
 
SDO was launched in February 2010. The satellite is orbiting the Earth in a circular, geosynchronous orbit at an altitude of 36,000 kilometres. It monitors constantly solar variations so scientists can understand the cause of the change and eventually have a capability to predict the space weather.

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