W., Hill, F., Hubbard, R

Harvey, J · 1996

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astro-ph.SR · 2026-04-13 · unverdicted · novelty 5.0

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 signatures in the Fraunhofer G-band; Testing ionization memory with multi-line prominence diagnostics astro-ph.SR · 2026-04-13 · unverdicted · none · ref 7
Prominence emission in the G-band originates from Ti II and Ca I lines, not CH, and shows no clear ionization memory effect.