Fine Scale Structure in Cometary Dust Tails - Figure 5.24 - Solar Wind adjust...
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Three solar wind aligned temporal maps of C/2011 L4's main dust tail region as seen by HI-1B with coarse-scale difference enhancement. The x-axis corresponds to the paths...
由HI-1B拍摄并经粗尺度差分增强处理的三张与太阳风方向对齐的C/2011 L4彗星主尘埃尾区域时序图像，横轴对应于运动路径……
