In this paper , we present a detailed analysis of a coronal blowout jet eruption which was associated with an obvious extreme-ultraviolet ( EUV ) wave and one complicated coronal mass ejection ( CME ) event based on the multi-wavelength and multi-view-angle observations from Solar Dynamics Observatory and Solar Terrestrial Relations Observatory .
It is found that the triggering of the blowout jet was due to the emergence and cancellation of magnetic fluxes on the photosphere .
During the rising stage of the jet , the EUV wave appeared just ahead of the jet top , lasting about 4 minutes and at a speed of 458 - 762 km s ^ { -1 } .
In addition , obvious dark material is observed along the EUV jet body , which confirms the observation of a mini-filament eruption at the jet base in the chromosphere .
Interestingly , two distinct but overlapped CME structures can be observed in corona together with the eruption of the blowout jet .
One is in narrow jet-shape , while the other one is in bubble-shape .
The jet-shaped component was unambiguously related with the outwardly running jet itself , while the bubble-like one might either be produced due to the reconstruction of the high coronal fields or by the internal reconnection during the mini-filament ejection according to the double-CME blowout jet model firstly proposed by Shen et al .
( 2012b ) , suggesting more observational evidence should be supplied to clear the current ambiguity based on large samples of blowout jets in future studies .