Fine Scale Structure in Cometary Dust Tails - Figure 5.23 - Solar Wind adjust...
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Three solar wind aligned temporal maps of McNaught's main dust tail region as seen by HI-1A with MGN enhancement.The x-axis corresponds to the paths through the comet tail taken...
由HI-1A观测得到并经MGN增强处理的三组与太阳风对齐的麦克诺特彗星主尘埃尾区域时序映射图，其x轴对应穿过彗星尾部的观测路径……
