The Tiny Physics Behind Immense Cosmic Eruptions

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The Tiny Physics Behind Immense Cosmic Eruptions
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A new theory describes how particle interactions fuel fast magnetic reconnection, the process behind solar flares and other astrophysical jets.

proposes that when it comes to solving the mysteries of magnetic reconnection, tiny physics plays a big role. In particular, it explains why some reconnection events are so stupefyingly fast—and why the strongest seem to occur at a characteristic speed. Understanding the microphysical details of reconnection could help researchers build better models of these energetic eruptions and make sense of cosmic tantrums., a plasma physicist at Princeton University who was not involved in the study.

In the 1950s, scientists proposed an explanation for how plasmas eject their pent-up energy, a process that came to be called magnetic reconnection. When magnetic field lines pointing in opposite directions collide, they can snap and cross-connect, launching particles like a double-sided slingshot. But this idea was closer to an abstract painting than a complete mathematical model. Scientists wanted to understand the details of how the process works—the events that influence the snapping, the reason why so much energy is unleashed. But the messy interplay of hot gas, charged particles and magnetic fields is tricky to tame mathematically., described in 1957 by the astrophysicists Peter Sweet and Eugene Parker, treats plasmas as magnetized fluids.

But solar flares release energy much more quickly than Sweet and Parker’s theory can account for. By their calculations, those flares should unfurl over months rather than minutes.identified this speedier reconnection happening even closer to home, in Earth’s own magnetic field.

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