Emission proxy images for the cooler temperature range (30 000 − 300 000 K) for the first eruption at t = 285.8 min (left column) and the second eruption at t = 320.1 min (right column). The upper, middle, and lower panels correspond to integrating over the x, y, and z lines of sight, respectively. The B_z magnetic field contours at the photosphere are overlaid in the lower panel.