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Fig. 1.

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Evolution of the jet observed by EUVI on board STA and STB and radio bursts observed by STA/WAVES. (a): STA/WAVES observations of two interplanetary type-III radio bursts as well as a weak and short-lived type-II radio burst, marked by white arrows. (b)–(d): observations of the jet at ∼21:06 UT from STB/EUVI 195 Å, STA/EUVI, and STB/EUVI 304 Å, respectively. The source region is marked by a white box in panel (d). (e)–(g): jet observations at ∼21:16 UT from STB/EUVI 195 Å, STA/EUVI, and STB/EUVI 304 Å. Two running-ratio images (with respect to the previous images) in panels (b) and (e) are chosen to enhance the signal-to-noise of the jet. (h): EUV wave on the disk at ∼21:10 UT in STA/EUVI 195 Å.

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