例句與造句

1. And there are no hard-core pressure tactics once they've signed on.
2. Inner-core pressures are more than 3 million times greater than those at the earth's surface.
3. The population of positrons provides a brief reservoir of new gamma rays as the expanding supernova's core pressure drops.
4. During core hydrogen burning, the helium fraction in the core increases and according to the virial theorem the core pressure and temperature will increase.
5. Its core pressure ultimately fell to 966 mbar by 00 : 00 UTC the next day, while located off the coast of southwestern Nova Scotia.
6. It's difficult to find core pressure in a sentence. 用core pressure造句挺難的
7. At an early stage of the project, the overall pressure ratio was 27 : 1 with a core pressure ratio of " over 17 ".
8. In a collection of hcp crystals at inner-core pressures, the computer calculations showed, seismic waves would travel faster perpendicular to the hexagonal planes than parallel to them.
9. But no one knew what the speed of sound in iron was at inner-core pressures, let alone what particular crystal structure might explain the speed differences observed by seismologists.
10. Maybe if a star becomes too massive, the core pressure forces the density into a black hole perhaps ? talk ) 22 : 30, 30 July 2008 ( UTC)
11. Another criterion for separating planets and brown dwarfs, rather than deuterium fusion, formation process or location, is whether the core pressure is dominated by coulomb pressure or electron degeneracy pressure.
12. Another criterion for separating planets and brown dwarfs, rather than deuterium burning, formation process or location, is whether the core pressure is dominated by coulomb pressure or electron degeneracy pressure.
13. I forget what I calculated the core pressure to be for this model, but it's no more than 1000GPa, whereas the pressure necessary for fusion is nearly 1000 times that.
14. This results in a decrease in pressure support, which causes the core to contract until the increased density and temperature bring the core pressure into equilibrium with the layers above.
15. Other experimental studies show a discrepancy under high pressure : diamond anvil ( static ) studies at core pressures yield melting temperatures that are approximately 2000 K below those from shock laser ( dynamic ) studies.
16. If you equate the effective pressure of the outgoing radiation as a function of the distance to the black hole, to the core pressure in the Sun you get an estimate of the radius of the bubble around the black hole that the Hawking radiation creates.