A new optimization method using contribution functions and non-LTE modeling generates plasma parameter maps from dual Lyman line intensities in solar prominences.
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Prominence emission in the G-band originates from Ti II and Ca I lines, not CH, and shows no clear ionization memory effect.
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Prominence Plasma Parameters Maps Inferred From Lyman $\beta$ and Lyman $\gamma$ Observations and Non-LTE Modelling
A new optimization method using contribution functions and non-LTE modeling generates plasma parameter maps from dual Lyman line intensities in solar prominences.
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Prominence signatures in the Fraunhofer G-band; Testing ionization memory with multi-line prominence diagnostics
Prominence emission in the G-band originates from Ti II and Ca I lines, not CH, and shows no clear ionization memory effect.