(June 28, 2015) Mathematicians at the University of Sheffield, as part of an international team, have discovered tornadoes in space which could hold the key to power the atmosphere of the Sun to millions of kelvin.
The super tornadoes - which are thousands of times larger and more powerful than their earthly counterparts but which have a magnetic skeleton - spin at speeds of more than 6,000 mph at temperatures in millions of centigrade in the Sun’s atmosphere.
They are more than 1,000 miles wide – hundreds of miles longer than the total distance between Land’s End to John O’Groats. It is estimated that there are as many as 11,000 of these swirling events above the Sun’s surface at any time.
Applied mathematicians from the University of Sheffield (Professor Robertus Erdélyi –senior author, and Dr Viktor Fedun) collaborating with the University of Oslo in Norway (Drs Sven Wedemeyer-Böhm – first author, Eamon Scullion – a Sheffield ex-postgraduate, Luc Rouppe van de Voort), Kiepenheuer Institute for Solar Physics of Freiburg, Germany (Dr Oskar Steiner), and Uppsala University in Sweden (Jaime de la Cruz Rodriguez), say the solar tornadoes carry the energy from the energy reservoir below the Sun’s surface, called the convection zone, to the outer atmosphere in the form of magnetic waves.