Abstract:<p><em>Context</em>: Magnetic switchbacks are localised polarity reversals in the radial component of the heliospheric magnetic field. Observations from <em>Parker Solar Probe </em>(PSP) have shown that they are a prevalent feature of the near-Sun solar wind. However, observations of switchbacks at 1 au and beyond are less frequent, suggesting that these structures are dissipated by yet-to-be identified mechanisms as they propagate away from… Show more
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