用WMAP造句子，“WMAP”造句

這種扭曲以WMAP探測器温度數據漂移的形式表現出來，從而揭示出星系團的運動方向和速度。

他們指出WMAP的數據明顯顯示出在更小的角度尺度上具有更多的熱點和冷點，因此假設微波背景各向同*是錯誤的。

此外，通過對WMAP探測器數據中看到温度變化力度的X光亮度進行比較，該小組測試了他們的分析方法。

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.

而且，他確實識別出WMAP數據裏有一定數量的圓環具有明顯低於周圍背景的温度差。

在美宇航局的威爾金森微波各向異*探測器（WMAP）【3】所獲得的數據中，這個算法在宇宙中發現有四個地區，它們標記出有着良好的研究前景。

And indeed, he identified a number of rings within the WMAP data that had a temperature variance that was markedly lower than that of the surrounding sky.

但WMAP卻沒能夠發現這些高能量的光子，所以在宇宙微波背景輻*上那些星系的周圍有些光子的虧損。

Previously, scientists using data from WMAP measured the time since the Big Bang to be an incredibly precise 13.73 billion years (give or take 0.12 billion years).

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.

這則消息來自WMAP團隊公開發表的一系列論文，這是些涉及到不同觀測方向的論文。

WMAP cannot detect these higher energy photons, so there should be a deficit of CMB photons around clusters.