例句與造句

1. Direct-cool refrigerators produce the cooling effect by a natural convection process.
2. Due to the large temperature difference between the air exhausted and the ambiance air generates small-scale convection processes.
3. Iron rain as part of atmospheric convection processes is possible only in brown dwarfs, and not in small stars.
4. The distribution of energy from the rising hot water to the sinking cold water contributes to the convection process.
5. "' Marklund convection "', named after G鰎an Marklund, is a convection process that takes place in filamentary currents of plasma.
6. It's difficult to find convection process in a sentence. 用convection process造句挺難的
7. Both of these convection processes immediately begin to slow down, and eventually stop, as soon as the burners turn off.
8. The convection process also prevents surface temperatures from becoming too extreme as they sometimes do when dark colored solid mass surfaces receive direct sunlight.
9. :I always understood that the reason a full fridge required less power to maintain temperature was that an empty one lost more heat through convection processes.
10. This heat transfer creates a convection process inside of the empty space that is very similar to the one that takes place inside of the firebox.
11. However, some exceptionally energetic convection processes-- notably volcanic overshooting tops associated with severe supercell thunderstorms-- may " locally " and " temporarily " inject convection through the tropopause and into the stratosphere.
12. In stars, the convection process is known to be highly efficient, with a typical \ frac { d \ ln T } { d \ ln P } that only exceeds the adiabatic gradient by 1 part in 10 million.
13. "' Schmidt number "'( "'Sc "') is a dimensionless number defined as the ratio of momentum diffusivity ( viscosity ) and mass diffusivity, and is used to characterize fluid flows in which there are simultaneous momentum and mass diffusion convection processes.
14. The convection process could also account for the thorough mixing of heavy and light elements in supernova debris, particularly how elements known to form deep within a star could be in the outermost observable layers of an explosion, as was the case in SN1987A.