Our sun’s fiery flares are even more extreme than scientists had thought, blasting particles to temperatures six times hotter than earlier estimates, according to new research.
Solar flares are colossal explosions in the sun’s atmosphere that hurl out bursts of powerful radiation. These events are notorious for disrupting satellites, scrambling radio signals and potentially posing dangers to astronauts in space.
Now, a team led by Alexander Russell of the University of St. Andrews in Scotland reports that particles in the sun’s atmosphere heated up by flares can reach a staggering 60 million degrees Celsius (108 million degrees Fahrenheit) — tens of millions higher than earlier predictions, which typically put such temperatures between 10 million and 40 million degrees Celsius (18 million to 72 million degrees Fahrenheit).
“This appears to be a universal law,” Russell said in a statement. The effect has already been observed in near-Earth space, the solar wind and in simulations, he added, but until now, “nobody had previously connected work in those fields to solar flares.”
Since the 1970s, astronomers have been puzzled by a strange feature in the light from solar flares. When split into colors using powerful telescopes, the telltale “spectral lines” of different elements look much broader, or blurrier, than theory predicts.
For decades, scientists chalked this up to the turbulence known to occur in the sun’s plasma. Like the chaotic bubbling of boiling water, the swift, random motions of charged particles in plasma can, in theory, shift light in different directions as they move. But the evidence never fully matched up, the new study notes. Sometimes the broadening appeared before turbulence could form, and in many cases the shapes of the lines were too symmetrical to match turbulent flows, according to the paper.
In their new study, Russell and his team suggest a simpler explanation: the solar particles affected by flares are simply far hotter than previously thought.
Using experiments and simulations of magnetic reconnection — the snapping and realignment of magnetic field lines that powers flares — the researchers found that, while electrons may reach 10 million to 15 million degrees C (18 million to 27 million degrees C), ions can soar past 60 million degrees C (108 million degrees F). Because it takes minutes for electrons and ions (which are…
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