例句與造句

1. Over C魌e d'Ivoire, interferometrically recorded spectra of outgoing longwave radiation ).
2. Radiative cooling by outgoing longwave radiation is the primary way the Earth System loses energy.
3. Outgoing longwave radiation ( OLR ) has been monitored globally since 1975 by a number of successful and valuable satellite missions.
4. This cooling is offset somewhat by the greenhouse effect of clouds which reduces the outgoing longwave radiation by about 31 W / m?
5. Over 99 % of outgoing longwave radiation has wavelengths between 4 祄 and 100 祄, in the thermal infrared part of the electromagnetic spectrum.
6. It's difficult to find outgoing longwave radiation in a sentence. 用outgoing longwave radiation造句挺難的
7. Note that the last afd was a vote to Redirect to Outgoing longwave radiation . talk ) 22 : 46, 3 May 2016 ( UTC)
8. The first term is equal to the change in temperature due to incoming solar radiation and outgoing longwave radiation, which changes with time throughout the day.
9. At night, the absorptive effect of clouds on outgoing longwave radiation, such as heat energy from the surface, allows for warmer diurnal low temperatures in all seasons.
10. In 2000, a comparison between measurements and dozens of GCM simulations of ENSO-driven tropical precipitation, water vapor, temperature, and outgoing longwave radiation found similarity between measurements and simulation of most factors.
11. In the wavelength range between 4 祄 and 10 祄 the spectrum of outgoing longwave radiation overlaps that of solar radiation, and for various applications different cut-off wavelengths between the two may be chosen.
12. Over the Atlas Mountains, interferometrically recorded spectra of outgoing longwave radiation show emission that has arisen from the land surface at a temperature of about 320 K and passed through the atmospheric window, and non-window emission that has arisen mainly from the troposphere at temperatures about 260 K.
13. For planets with temperature-dependent sources of greenhouse gases such as liquid water and optically thin atmospheres the outgoing longwave radiation curve ( which indicates how fast energy can be radiated away by the planet ) flattens at high temperatures, reaching a horizontal asymptote  the Kombayashi Ingersoll limit itself.