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IR thermometry: then and now

机译:红外测温:过去和现在

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In 1800 William Herschel, the great astronomer and telescope maker, tried an experiment. Like Newton in 1666, he passed a beam of white light through a glass prism and found, spread out before him, the familiar spectrum of colours, from violet to red. Unlike Newton, he placed a thermometer at various points along the spectrum and, as he suspected, found that the temperatures differed. The lowest were at the violet end of the spectrum and they rose toward the red and then, beyond the end of the spectrum, they kept rising. Not only had Herschel proved what he had set out to prove (that light and radiant heat are identical, itself a momentous finding) but he had discovered infrared radiation extending beyond the end of the visible spectrum. As the great man noted, radiant heat consists of "invisible light".
机译:1800年,伟大的天文学家和望远镜制造商威廉·赫歇尔(William Herschel)进行了实验。像1666年的牛顿一样,他将一束白光穿过玻璃棱镜,发现在他面前散布着从紫罗兰色到红色的各种熟悉的色彩。与牛顿不同,他在光谱的各个点放置了温度计,并怀疑温度不同。最低的是在光谱的紫罗兰色末端,然后朝着红色上升,然后,在光谱的末端,它们一直在上升。赫歇尔不仅证明了他打算证明的事实(光和辐射热是相同的,本身就是一个重大发现),而且他发现了红外辐射超出了可见光谱的范围。正如伟人所指出的那样,辐射热由“不可见光”组成。

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