“反照率”造句

這些云帶必定引起行星反照率的經(jīng)向不對(duì)稱性.
These bands must introduce longitudinal asymmetry in the planetary albedo.

如果恒星的光譜已知, 就可得出塵埃的反照率.
If the stellar spectrum is known, the albedo of the dust can be obtained.

有云區(qū)也可能是輸射虧損區(qū),因?yàn)樵朴休^高的反照率.
Cloudy areas can also be areas of radiation deficit because of their higher albedo.

• #反照率