Column mass and temperature profile steepness dominate He II 304 Å line formation in the February 15 2022 eruptive prominence, with radiative processes outweighing collisional excitation.
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Analysis of Eruptive Prominence Plasma Parameters' Effects on the \ion{He}{2} 304~\AA\ Line with Solar Orbiter EUI Observations
Column mass and temperature profile steepness dominate He II 304 Å line formation in the February 15 2022 eruptive prominence, with radiative processes outweighing collisional excitation.