In 3D simulations, partial ionization makes emerging solar magnetic fields arch-like with little twist and produces faster ejective eruptions than the fully ionized case.
D., Haynes, M., & Leake, J
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Magnetic flux emergence and solar eruptions in partially ionized plasmas
In 3D simulations, partial ionization makes emerging solar magnetic fields arch-like with little twist and produces faster ejective eruptions than the fully ionized case.