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A discrete picture of magnetic fields in microquasar jets
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DOI：10.1038/s41550-026-02935-1.png)
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Abstract
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Sewn or knitted? State-of-the-art magnetohydrodynamic simulations offer an insight into how magnetic field topology might be shaped by the episodic nature of the relativistic ejections in the ‘clocked’ Galactic microquasar SS 433.
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