available temperature effective humidity effective temperature effective temprature effectivetemperature
Example Sentences:
1.
Effective accumulative temperature 有效温度总和
2.
Available temperature drop 有效温度下降
3.
Based on the analyses of velocity field and temperature field , with using valid - temperature - difference as evaluation target , the author calculates and analyzes the thermal comfort character of guest rooms 在对室内温度场、速度场分析的基础上，采用“有效温度差”作为评价指标，对客房的热舒适性进行计算、分析。
4.
The relation between stellar chromospheric activity and rotation of evolution stars have a good relativity . but meticulous analysis show chromospheric activity of evolution stars depend on stellar spectral type and effective temperature strongly . we provide several possible explain for those phenomena 但是细致分析显示演化恒星色球活动水平随恒星自转周期间的分布对恒星光谱型和恒星表面有效温度有很强的依赖，并对这些现象提出了几种可能的解释。
5.
Make the theoretical and experimental research of self - cleanup , through the experimental research to the tin , we get the conclusions of jointed cold - blowing and hot - blowing period and the effective temperature range etc . proposed the practical measures to improve the effect of the self - cleanup , laid the groundwork for the future further in - depth study and application 通过对蓄冷器的实验研究,掌握了冷吹期和热吹期的温度变化规律,获得了热吹期填料温度闭合和输出气流有效温度范围等结论。通过自清除原理的分析和自清除过程的实验,提出了改善自清除效果的实用措施,为今后进一步深入研究和应用打下了基础。
6.
The experimental results are helpful to understand the acceleration mechanisms of the hot electron emission in the interaction of the us - ui laser pulse with plasma . an anisotropy energy distribution of the hot electrons emiaon has been observed for the first time in the experiments . the energy spectrum of hot electrons resulted from the resonance absorption at the direction of target normal is a maxwellian - like distribution E11分布，拟合的超热电子有效温度约200kev左右，超热电子的最大能量约zmev ，加速电子的主导机制是共振吸收机制;反射方向超热电子的能谱在低能段出现一个局部的平台( pla1leau ) ，呈现出非类maxwen分布，这是几种加热机制共同作用的结果，其中占主导地位的是反射激光加速机制。
7.
Because the photospheric temperature of carbon stars are less than 3000k and the temperature of rich - dust envelope formed by the mass loss is lower , and therefore most of the energy from carbon stars are radiated between 1 to 60um range , in which the vibrational and ro - vibrational bands of many molecules also lies , the study of infrared spectra in this wavelength range is very important to reveal chemical compositions , dust formation process , the atmospheric structure and evolutionary status of stars 碳星光球的有效温度不超过3000k ，同时较大的质量损失率形成了富碳的尘埃壳层，以致于它的辐射能量主要集中在1 ? 60 m的红外波段上，并且许多分子的转动振动能谱也集中在红外，因此在红外波段的研究对揭示碳星化学成份及其分布、尘埃形成过程、恒星大气结构和演化状态都有十分重要的意义。
