Table 1.

Summary of EUV spectral line enhancements for M- and X-class flares. Values are percent increases relative to pre-flare background.

EUV Line Typical Enhancement (%) Extreme Enhancement (%)

M-class X-class M-class X-class
He II 30.4 nm 0.3–15 0.8–40 ∼30 65–78
Lyα 121.6 nm 0.5–5 0.1–7 27 10–12
Mg II 0.1–2 0.1–3 2.5 4–5

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