通过四阶方程拟合实验数据和热力学数据得到的稳定带厚度更接近实际情况；
The calculated thickness of stability zone by the four-order polynomial using the experiment and thermodynamics data is close to practice.
在色星等图上，处于造父不稳定带的左外侧而温度较高，故简称热造父变星。
On the colour-magnitude diagram they are situated near and more left than the hotter edge of the Cepheid instability stripe, so their temperature is higher than other types of pulsating variables.
海底温度和压力、地热梯度、气体成分、同生水盐度等控制着水合物稳定带基底的深度和厚度。
Submarine temperature, pressure, gas compositions, geothermal gradient and syngenetic water salinity control the depth of hydrate zone basement.
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