4.7 Article

Foreshock as a Source Region of Electron-scale Magnetic Holes in the Solar Wind at 1 au

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Summary: The coronal heating region can generate mirror mode structures that evolve into magnetic holes, with ion vortexes playing a crucial role in their formation. These magnetic holes can be transported long distances by the solar wind, with recent observations revealing the presence of ion vortexes inside them. Understanding the role of ion vortexes in shaping magnetic holes may provide insights into their long-term survival in astrophysical plasmas.

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