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Direct observation of turbulent magnetic reconnection in the solar wind - Nature Astronomy

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Direct observation of turbulent magnetic reconnection in the solar wind - Nature Astronomy

Magnetic reconnection in a current sheet is commonly found in astrophysical plasma environments. If it is often bursty, releasing magnetic free energy explosively, in planetary magnetospheres, it instead displays a quasi-steady state in the solar wind, where the energy is dissipated via slow-mode shocks. The reason for this difference is elusive.

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Direct observation of turbulent magnetic reconnection in the solar wind - Nature Astronomy

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Direct observation of turbulent magnetic reconnection in the solar wind - Nature Astronomy

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