• It takes the right combination of wind,temperature,pressure and humidity to create even a weak tornado.

    VOA: special.2010.05.11

  • That is, most processes that we're concerned with, they'll happen with something held constant like pressure or temperature or maybe volume.

    这句话是说我们所关注的大部分过程,发生的时候都是保持某个量为常数,比如压强,温度或者体积。

    麻省理工公开课 - 热力学与动力学课程节选

  • So this unique temperature and unique pressure defines a triple point everywhere, and that's a great reference point.

    这样,无论在何处,三相点都具有相同的温度和压强,十分适合来作参考点。

    麻省理工公开课 - 热力学与动力学课程节选

  • Mister Harrison had to develop a clock that was not affected by the movement of a ship on the ocean or changes in temperature or atmospheric pressure.

    VOA: special.2010.07.14

  • We could just collect a bunch of data. For a material .What's the volume it occupies at some pressure and temperature?

    对一种物质我们可以得到一系列测量数据,在给定的温度和气压下,它的体积是什么?

    麻省理工公开课 - 热力学与动力学课程节选

  • But we've defined the enthalpy of those elements in their stable state at room temperature and pressure as zero, right?

    但我们已经定义了这些,元素处于它们室温和常压下,最稳定的状态时的焓为零,对吧?

    麻省理工公开课 - 热力学与动力学课程节选

  • OK, now what we'd like to do is be able to calculate any of these quantities in terms of temperature, pressure, volume properties.

    现在我们想要做的是能够利用,温度,压强和体积的性质,计算上面的物理量。

    麻省理工公开课 - 热力学与动力学课程节选

  • On the other hand, temperature, volume and pressure are variables that are much easier in the lab to keep constant.

    另一方面,温度,体积和压强,在实验室中比较容易保持恒定。

    麻省理工公开课 - 热力学与动力学课程节选

  • What we define as zero is the enthalpy of every element in its natural state at room temperature and ambient pressure.

    我们将零点定义为每种元素,在室温和正常大气压下,在其自然状态下的焓。

    麻省理工公开课 - 热力学与动力学课程节选

  • And the equation of state, pressure versus volume at constant temperature, is going to have some form, let's just draw it in there like that.

    系统的态函数,恒温下压强比体积,变化曲线,就像这样。

    麻省理工公开课 - 热力学与动力学课程节选

  • are all functions of state and parameters that we can control like temperature and pressure.

    公式里面的全部都是态函数,我们控制态函数的参数比如温度或者压强。

    麻省理工公开课 - 热力学与动力学课程节选

  • Whereas under these conditions, these quantities, if you look at free energy change, for example at constant temperature and pressure, H you can still calculate H.

    但是,在这些条件下,这些物理量,如果我们考察自由能的变化,例如在恒定的温度和压强下,我们仍然可以计算。

    麻省理工公开课 - 热力学与动力学课程节选

  • Hydrogen gas it's in its most stable state, right at room temperature and pressure.

    和常压下氢气是氢元素,最稳定的状态,这个小“0“

    麻省理工公开课 - 热力学与动力学课程节选

  • For instance, the pressure and the temperature, or the volume and the pressure.

    比如压强和温度,或体积和压强。

    麻省理工公开课 - 热力学与动力学课程节选

  • It's a state function, so we're at constant temperature and pressure, and now we want to consider some chemical change or a phase transition or you name it.

    这就是态函数,我们处于恒定的温度和压强之下,然后考虑某些化学变化或者相变,或者你想考虑的东西。

    麻省理工公开课 - 热力学与动力学课程节选

  • There's a volume, there's a temperature, than the pressure here. There's other volume, temperature and pressure here, corresponding to this system here.

    温度等状态函数有本质区别,这个状态有一组,确定的体积,温度与压强。

    麻省理工公开课 - 热力学与动力学课程节选

  • And so, again, we see a temperature increase, and we know the work, and the temperature increase, it's a constant pressure thing.

    好,我们看到温度升高了,然后我们有做功量和温度的升高量,这是一个恒定压力下的值。

    麻省理工公开课 - 热力学与动力学课程节选

  • So, all I want to do now is look at the derivatives of the free energies with respect to temperature and volume and pressure.

    我现在所要做的一切就是,考察自由能对,温度,体积和压强的偏导数。

    麻省理工公开课 - 热力学与动力学课程节选

  • And I didn't specify the conditions, but if we were to do this under ordinary chemical conditions of some, you'd say room temperature and pressure, right, they all happen spontaneously.

    我并没有特别说明反应条件,但是如果我们在通常的化学条件下,实现这些化学反应,比如在室温和大气压下下,他们都是自发的。

    麻省理工公开课 - 热力学与动力学课程节选

  • And you can find these compressibility factors in tables. If you want to know the compressibility factors for water, for steam, at a certain pressure and temperature, you go to a table and you find it.

    各种气体的压缩系数,想知道水或者水蒸气,在某个温度和压强下的,压缩系数,查表就行了,这是实际气体状态方程的。

    麻省理工公开课 - 热力学与动力学课程节选

  • So again with the Gibbs free energy, now I see how to determine, if I change the pressure, if I change the temperature by some modest amount, how much is the Gibbs free energy going to change?

    再一次通过吉布斯自由能,我知道当我,适当的改变压强和,温度的时候,吉布斯自由能如何变化?

    麻省理工公开课 - 热力学与动力学课程节选

  • Now in this particular reaction, I've got hydrogen gas, iron solid. Those already are elements in their most stable forms at room temperature and pressure.

    特定的反应中,我有氢气,固态铁,这些都已经是,处于室温和常压下,最稳定的元素单质。

    麻省理工公开课 - 热力学与动力学课程节选

  • And this volume, temperature and pressure doesn't care how you got there. It is what it is.

    另一个状态,也有一组确定的体积。

    麻省理工公开课 - 热力学与动力学课程节选

  • We know how the volume and temperature vary with respect to each other at constant pressure.

    知道在恒定压强下,体积如何随着温度变化。

    麻省理工公开课 - 热力学与动力学课程节选

  • Because so much of what we do in chemistry does take place with constant temperature and pressure.

    因为化学中我们所做的很多东西,都是在恒定的温度和压强下进行的。

    麻省理工公开课 - 热力学与动力学课程节选

  • That is, it's easy to write down straight away that dG with respect to temperature at constant pressure S is minus S.

    这就是说,可以很简单的写出dG在,恒定压强下对温度的偏导数,是负。

    麻省理工公开课 - 热力学与动力学课程节选

  • You know how pressure changes with temperature at constant volume if you know the equation of state.

    如果你知道状态方程,知道在体积恒定的时压强如何随着温度变化。

    麻省理工公开课 - 热力学与动力学课程节选

  • There's our condition for equilibrium at constant temperature and pressure.

    这就是我们在,恒定温度和压强下的平衡条件。

    麻省理工公开课 - 热力学与动力学课程节选

  • You just need a few macroscopic variables that are very familiar to you, like the pressure, the temperature, the volume, the number of moles of each component, the mass of the system.

    你只需要某些你非常熟悉的宏观变量,比如压强,温度,体积,每个组分的摩尔数,系统的质量。

    麻省理工公开课 - 热力学与动力学课程节选

  • OK, you use the ideal gas law, etc., then you get a relationship that connects the pressure and the temperature, like here we got a relationship that connected the temperatures and the volumes together.

    我们会得到,一个联系初末态,的压强和温度的,关系式,就像这个联系过程中。

    麻省理工公开课 - 热力学与动力学课程节选

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