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Turbulent magnetic reconnection generated by intense lasers - Nature Physics

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Turbulent magnetic reconnection generated by intense lasers - Nature Physics

Turbulent magnetic reconnection is believed to occur in astrophysical plasmas, and it has been suggested to be a trigger of solar flares. It often occurs in long stretched and fragmented current sheets. Recent observations by the Parker Solar Probe, the Solar Dynamics Observatory and in situ satellite missions agree with signatures expected from turbulent reconnection.

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Turbulent magnetic reconnection generated by intense lasers - Nature Physics

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Turbulent magnetic reconnection generated by intense lasers - Nature Physics

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