“反照”造句
这些云带必定引起行星
反照率的经向不对称性.
These bands must introduce longitudinal asymmetry in the planetary albedo.
如果恒星的光谱已知, 就可得出尘埃的
反照率.
If the stellar spectrum is known, the albedo of the dust can be obtained.
有云区也可能是输射亏损区,因为云有较高的
反照率.
Cloudy areas can also be areas of radiation deficit because of their higher albedo.