1D multi-fluid MHD models show inverse FIP effect can arise for upward Alfvén waves when magnetic field strength and flux-tube expansion counteract multi-fluid dissipation and damping.
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Observational evidence points to the chromosphere as the site of chemical fractionation responsible for the FIP effect in the solar corona.
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Multi-fluid multi-species models for inverse FIP-effect
1D multi-fluid MHD models show inverse FIP effect can arise for upward Alfvén waves when magnetic field strength and flux-tube expansion counteract multi-fluid dissipation and damping.
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The connection between solar coronal abundances and the underlying lower atmospheric properties
Observational evidence points to the chromosphere as the site of chemical fractionation responsible for the FIP effect in the solar corona.