温度的记录间的细微差别的原因还有一点是不同研究所运用的测量温度的参考不一样。

The temperature records also differ slightly because the point of reference that each group uses to calculate global temperature is different.

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利用1857颗恒星的光线，一个由来自法国和美国天文学家组成的研究小组通过测量星光之间的细微差距来测定太阳周围气体的密度。

Using the light from 1, 857 stars, a team of French and American astronomers were able to measure the density of the gas surrounding our sun by examining fine differences in the starlight.

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根据亮场和暗场的正向曲线来计算的，通常情况下得到一个稍微较小的测量值，因为二极管效应在亮场和暗场条件下有稍微差异的。

Calculated from the light - and dark-forward curve, usually gives you values that are slightly too low because the diode curves from the light and dark measurements are slightly different.

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