Now, new data from the Hinode (Japanese for sunrise) satellite shows "magnetic waves" in the charged particles swirling around in the Sun play a critical role in driving the solar wind into space, according to studies by international researchers published in the journal Science.
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The magnetic waves, called Alfvén waves after the Swedish scientist who suggested them in 1942, ripple in the electrically charged gas of particles - plasma - within the Sun and its atmosphere.
They have always been a leading candidate in the formation of solar wind since they can transfer energy for the wind from the Sun's surface up through its atmosphere.
"Until now, Alfvén waves have been impossible to observe because of limited resolution of available instruments," said Alexei Pevtsov, Hinode program scientist, at Nasa Headquarters, Washington.
"With the help of Hinode, we are now able to see direct evidence of Alfvén waves, which will help us unravel the mystery of how the solar wind is powered."
Using Hinode's high resolution X-ray telescope, a team led by Jonathan Cirtain at Nasa's Marshall Space Flight Centre, Huntsville, Alabama, peered into the atmosphere at the Sun's poles and observed record numbers of jets of X-rays, sent out as fountains of rapidly-moving hot plasma.
Cirtain's team observed an average of 240 jets per day, some up to 12,000 miles wide and 600,000 miles long, and conclude that Alfvén waves are being formed at the same time.
"The large number of jets, coupled with the high speeds of the outflowing plasma, lends further credence to the idea that X-ray jets are a driving force in the creation of the fast solar wind."