Fig. 5.
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Temporal evolution at selected wavelengths. From top to bottom: GOES soft X-rays 1–8 and 0.5–4 Å, EOVSA 8 GHz, AR30T mid-IR (30 THz), AIA 1700 Å and HASTA Hα. The error bar shown at the top left of the 30 THz plot corresponds to 1σ uncertainty in ΔTb. The sharp peak visible in the 8 GHz curve during the impulsive phase of the flare extends up to ∼3 SFU. SFU = solar flux unit.
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