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Transient Inverse-FIP Plasma Composition Evolution within a Confined Solar Flare

By Deborah Baker and others
Understanding elemental abundance variations in the solar corona provides an insight into how matter and energy flow from the chromosphere into the heliosphere. Observed variations depend on the first ionization potential (FIP) of the main elements of the Sun's atmosphere. High-FIP elements (>10 eV) maintain photospheric abundances in the corona,... Show more
February 19, 2019
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Transient Inverse-FIP Plasma Composition Evolution within a Confined Solar Flare
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