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A 50-year-old enigma has been solved! A new study reveals that the strange width of spectral lines in solar flares is not due to turbulence, but because ions are heated 6.5 times more than electrons. The Sun continues to reveal its secrets!
#Science #Sun #Astrophysics #MysterySolved

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00:0050-Year Solar Mystery Solved
00:02The incredible secret behind the sun's flares
00:06Since the 1970s, an enigma has baffled solar scientists
00:11The strange width of spectral lines during solar flares
00:15For decades, it was thought that this expansion was caused by turbulent motions in the solar plasma
00:21However, this explanation never quite fit
00:25Leaving a large gap in our understanding of how solar flares truly work
00:29But now, after 50 years, a new study from the University of St. Andrews has revealed a surprising solution
00:37Solar flares are violent events that release enormous amounts of energy
00:41Heating the sun's outer atmosphere to more than 10 million degrees Celsius
00:46These explosions not only bombard Earth with radiation
00:50But they also give us clues about the physics of stars
00:53One of the biggest mysteries has been the unusual width of the spectral lines
00:58Those light signatures that the plasma emits during flares
01:03The turbulence theory never fully explained the phenomenon
01:06And the problem persisted for half a century
01:09The key to solving this enigma came from a change in perspective
01:13Historically, scientists assumed that the ions and electrons within the plasma had the same temperature
01:20However, the research team led by Dr. Alexander Russell discovered something fundamental
01:25The magnetic reconnection process
01:28Responsible for heating the plasma
01:31Heats ions 6.5 times more than electrons
01:35Although this phenomenon had already been observed near Earth and in the solar wind
01:40It had never been linked to solar flares
01:42By redoing the calculations with this new understanding
01:47The team realized that the incredibly high temperatures of the ions persist for minutes in the most crucial parts of the flares
01:53What was previously attributed to turbulence is now largely explained by the extreme heat of these ions
02:01This new view fits perfectly with observations and offers an unexpected and convincing solution to a 50-year-old mystery
02:09This discovery is a reminder that sometimes
02:12The key to solving great mysteries is not in seeking new answers
02:16But in re-evaluating old assumptions
02:18The sun, our closest star, continues to surprise us
02:23Revealing its secrets, ion by ion
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