Magnetic reconnection resulting from flux emergence: implications for jet formation in the lower solar atmosphere?

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Fig. 3

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Re-plot of the state at t = 80 s in Fig. 2a. The temperature is shown in a smaller color scale than in Fig. 2a. The two solid lines (black) denote the x-position of the slit, and P1 and P2 denote the two y-position of the slit.

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