Researchers
at Queen's University Belfast uncover some of the mysteries in how the sun able
to heat its atmosphere. The research article was published in “a study in
Nature Physics”
In that
article they reveal that magnetic waves crashing through the sun are one of the
main reasons for the heating process and thus propelling the sun wind.
The waves
play a important role in maintaining the sun’s super high temperatures, this
was predicted some 75 years ago now only it was proved.
"At
Queen's, we have now led a team to detect and pinpoint the heat produced by
Alfvén waves in a sunspot," Jess added. "This theory was predicted
some 75 years ago but we now have the proof for the very first time. Our
research opens up a new window to understanding how this phenomenon could potentially
work in other areas such as energy reactors and medical devices."
To find
the mystery, the research took advanced high-resolution observations from the
Dunn Solar Telescope in New Mexico, US, alongside complementary observations
from NASA's Solar Dynamics Observatory, to analyse the strongest magnetic
fields that appear in sunspots.
"By
breaking the sun's light up into its constituent colours, our international
team of researchers were able to examine the behaviour of certain elements from
the periodic table within the sun's atmosphere, including calcium and
iron," added another researcher on the paper, Dr. Samuel Grant from
Queen's University.
"Once
these elements had been extracted, intense flashes of light were detected in
the image sequences."
He said
that these intense flashes had all the hallmarks of the Alfvén waves converting
their energy into shock waves, in a similar way to a supersonic aircraft
creating a boom as it exceeds the speed of sound.
"The
shock waves then ripple through the surrounding plasma, producing extreme heat.
Using supercomputers, we were able to analyse the data and show for the first
time in history that the Alfvén waves were capable of increasing plasma
temperatures violently above their calm background," he explained.
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