A collisionless, low- plasma undergoing strong sub-Alfvénic turbulence is expected to form a broad hierarchy of reconnecting current sheets immersed in a strong guide magnetic field. If the reconnecting field strength of a sheet scales with its length as a power law of index , and the number of sheets per unit interval of sheet length decreases as a power law of index , the current-sheet ensemble injects nonthermal particles with a power-law energy spectrum , where . The spectrum is hard () when the longest sheets deliver most of the injected energy, which requires . Past numerical studies have measured , and the scalings of intense current sheets support , resulting in . This injection may yield flat or mildly steep radio spectra in optically thin sources and hard ion spectra in the coronae of active galactic nuclei.

生成讲解博客的中文版本

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