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一旦冲突被检测出来，它们可即时切换到未用频谱的备份频段。
When a conflict is detected, they switch to a backup slice of unused spectrum on the fly.
因为每隔90秒望远镜阵列就会切换观测另外一个星体或者一个不同的频段，一幅新的信息转换成的图像就会显示出来。
Every 90 seconds, the array switches to looking at a different star, or a different frequency range, and a new image is generated.
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