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Spacecraft Captures the "Magnetic Avalanche" that Triggers Giant Solar Explosions

Solar Orbiter’s high-resolution data reveal a 40-minute magnetic reconnection cascade driving the flare, accelerating particles to up to 50% the speed of light, key for space weather prediction.

  • On January 21, the ESA-led Solar Orbiter spacecraft revealed that initially weak magnetic disturbances triggered a flare via an avalanche-like cascade recorded on 30 September 2024, unveiling the flare's central engine.
  • Close-Up images showed new magnetic strands appeared nearly every image frame, roughly every two seconds, as the Extreme Ultraviolet Imager began observing at 23:06 UT, triggering rapid reconnections.
  • At 23:29 UT a brightening preceded the filament's detachment and violent unrolling, while X-ray emission surged around 23:47 UT accelerating particles to 40–50% of light speed and producing raining plasma blobs.
  • High-Energy X-ray mapping revealed accelerated particles deposited energy in the upper atmosphere, with reconnection events heating plasma and aiding predictions to protect satellites, aircraft and astronauts.
  • These findings challenge existing theories and support the avalanche model, while Miho Janvier and David Pontin call for future high-resolution X-ray missions to refine flare understanding.
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Science broke the news in on Wednesday, January 21, 2026.
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