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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Stokes V amplitude asymmetries are proposed as an alternative diagnostic for wave activity linked to FIP bias 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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Spectropolarimetric analysis of waves linked to FIP
Stokes V amplitude asymmetries are proposed as an alternative diagnostic for wave activity linked to FIP bias in the solar corona.