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.<\/p>\n
Solar flares<\/a> 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<\/a> and potentially posing dangers to astronauts in space.<\/p>\n <\/p>\n Now, a team led by Alexander Russell of the University of St. Andrews in Scotland reports that particles in the sun’s atmosphere<\/a> heated up by flares can reach a staggering 60 million degrees Celsius (108 million degrees Fahrenheit) \u2014 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).<\/p>\n You may like<\/p>\n “This appears to be a universal law,” Russell said in a statement<\/a>. The effect has already been observed in near-Earth space, the solar wind<\/a> and in simulations, he added, but until now, “nobody had previously connected work in those fields to solar flares.”<\/p>\n 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.<\/p>\n For decades, scientists chalked this up to the turbulence<\/a> 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.<\/p>\n 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.<\/p>\n Using experiments and simulations of magnetic reconnection<\/a> \u2014 the snapping and realignment of magnetic field lines that powers flares \u2014 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 atoms or molecules with an electrical charge) to share their heat, this temperature gap lasts long enough to shape the behavior of flares, according to the study.<\/p>\n At such extreme temperatures, ions zip around so quickly that their motion naturally makes the spectral lines look wider, “potentially solving an astrophysics mystery that has stood for nearly half a century,” Russell said in the statement.<\/p>\n The finds are not merely an academic exercise; they also carry implications for predicting space weather<\/a>. If scientists have been underestimating the energy stored in flare ions, forecasts of space weather may need to be revised. Improved models could give satellite<\/a> operators, airlines and space agencies more accurate information and extra time to prepare for dangerous solar events, scientists say.<\/p>\n The research also calls for a new generation of solar models, ones that treat ions and electrons separately instead of assuming a single uniform temperature. This “multi-temperature” approach is already common in other plasma environments, such as Earth’s magnetic field<\/a>, but has rarely been applied to the sun<\/a>, the study notes.<\/p>\n