SPICE spectra of Lyman lines in a solar prominence reveal intensity and width variations indicating evolving density, temperature, and optical depth, while a geometric model from paired H-alpha images yields the radial velocity during early eruption.
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Analysis of Lyman-beta and Lyman-gamma Lines in a Pre-Eruptive and Eruptive Prominence with Solar Orbiter SPICE Observations
SPICE spectra of Lyman lines in a solar prominence reveal intensity and width variations indicating evolving density, temperature, and optical depth, while a geometric model from paired H-alpha images yields the radial velocity during early eruption.