在2003年，美国航空航天局的威尔金森微波各向异性探测器绘制出了一幅空前详细的早期微波天空的地图，也是第一张完整的地图。
In 2003 NASA's Wilkinson microwave Anisotropy Probe produced the first full map of the early microwave sky in unprecedented detail.
从威尔金森微波各向异性探测器(WMAP)得来的数据显示出，细微温度变化是在宇宙微波背景辐射移动通过银河星系团气体时产生的。
Data from the Wilkinson microwave Anisotropy Probe (WMAP) can show the minute temperature changes created as the cosmic microwave background radiation moves through gases in galaxy clusters.
从欧洲航天局在2009年发射的普朗克卫星【4】所取得的数据有希望比从威尔金森微波各向异性探测器(wmap)的数据更为详细。
Data from the European Space Agency's Planck satellite, which launched in 2009, are expected to be far more detailed than those from WMAP.
在美宇航局的威尔金森微波各向异性探测器(WMAP)【3】所获得的数据中，这个算法在宇宙中发现有四个地区，它们标记出有着良好的研究前景。
In data from NASA's Wilkinson Microwave Anisotropy Probe (WMAP), the program found four regions in the universe that were flagged as promising.
之后的2003年，NASA在太空中的“威尔金森微波各向异性探测器”（WMAP）为穿越天空的CMB绘制了映射图，为早期宇宙制做了一幅精确的照片。
Then in 2003, NASA's space-based Wilkinson Microwave Anisotropy Probe (WMAP) mapped the CMB across the sky, producing an exquisite baby picture of the cosmos.
之后的2003年，NASA在太空中的“威尔金森微波各向异性探测器”（WMAP）为穿越天空的CMB绘制了映射图，为早期宇宙制做了一幅精确的照片。
Then in 2003, NASA's space-based Wilkinson Microwave Anisotropy Probe (WMAP) mapped the CMB across the sky, producing an exquisite baby picture of the cosmos.
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