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单词 Blackbody Spectrum
释义

Blackbody Spectrum

中文百科

黑体 (物理学) Black body

（重定向自Blackbody Spectrum）
当黑体的温度降低时，黑体辐射曲线峰值会移向较低强度和更长波长的位置。黑体辐射曲线图可以和经典模型瑞利-金斯定律相比较。
黑体辐射的颜色（色度）设根据黑体的温度变化的；这些颜色的轨迹，如上面的CIE1931色彩空间图所示，为普朗克轨迹（或称为黑体轨迹）。

在热力学中，黑体（英语：Black body），旧称绝对黑体，是一个理想化的物体，它能够吸收外来的全部电磁辐射，并且不会有任何的反射与透射。随着温度上升，黑体所辐射出来的电磁波与光线则称做黑体辐射。这个名词在1862年由克希荷夫所提出并引入热力学内。

英语百科

Black body 黑体 (物理学)

（重定向自Blackbody Spectrum）
As the temperature of a black body decreases, its intensity also decreases and its peak moves to longer wavelengths. Shown for comparison is the classical Rayleigh–Jeans law and its ultraviolet catastrophe.
An approximate realization of a black body as a tiny hole in an insulated enclosure
An idealized view of the cross-section of a star. The photosphere contains photons of light nearly in thermal equilibrium, and some escape into space as near-black-body radiation.
Effective temperature of a black body compared with the B-V and U-B color index of main sequence and super giant stars in what is called a color-color diagram.[36]

A black body is an idealized physical body that absorbs all incident electromagnetic radiation, regardless of frequency or angle of incidence. A white body is one with a "rough surface [that] reflects all incident rays completely and uniformly in all directions."
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更新时间：2025/6/22 8:24:19