黑体辐射的光谱分配由普朗克定律描述。
The spectral distribution of a black body radiation is described by planck's.
正常流态的光谱能量密度和辐射压强都比普通黑体大并且随温度单调增加。
Both spectral energy density and radiation pressure of the normal fluid are larger than those of the normal blackbody, furthermore, they are monotonically increasing functions of temperature.
正常流态的光谱能量密度和辐射压强都比普通黑体大并且随温度单调增加。
Both spectral energy density and radiation pressure of the normal fluid are larger than those of the normal blackbody, furthermore, they are monotonically increasing functions of temperature.
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