Chinese translation for "大气结构"

atmospheric structure

Related Translations:

大气:  1.(地球周围的气体) atmosphere; air2.(呼吸; 沉重的呼吸) breath; heavy breathing 短语和例子跑得直喘大气 breathe heavily from running; 吓得连大气也不敢出 catch or hold one's breath in fear

大气干燥:  air seasoning；air dryingatmospheric drying

爆炸性大气:  explosive atmosphere

大气氯:  atmo heric chlorineatmospheric chlorine

大气骚动:  

月球大气:  lunar atmosphere

自由大气:  

座舱大气:  aircraft cabin atmospherecabin atmosphere

扰动大气:  disturbd atmosphererough atmosphere

大气窗口:  atmospheric windows

Example Sentences:

	1.	Because biosphere 2 is a closed system , rainfall and aimospheric makeup can be regulated and measured , a1lowng scientists to conduct controlled experiments 因为生物圈2号是一个封闭的系统，所以降雨和大气结构都可以被调节和测量，以利于科学家做控制性实验。
	2.	For months , scientists have treated the city like a laboratory , testing wind patterns and atmospheric structure , while pinpointing local and regional pollution sources 一连好几个月，科学家将整个城市当作实验室，测试风的形态和大气结构，查明市内和市外的各种污染源。
	3.	Solar activity , especially , coronal mass ejection ( cme ) during a large solar activity affected the space environment of human being and could be one of main reasons of the space disaster 太阳活动密切地影响着日地空间环境和地球高空大气结构，太阳耀斑爆发产生的日冕物质抛射( cme )是空间灾害的主要原因之一。
	4.	And we also make the simulation of space - to - ground optical propagation by using the software of matlab , including scintillation , turbulent structure constant of atmosphere and spot of horizontal optical propagation 并用matlab语言实现了对空-地激光传输的光功率闪烁、大气结构常数以及湍流大气中的水平激光传输远场光斑的计算机模拟仿真。
	5.	Throughout the descent , shifts in the frequency of the probe ' s radio signal will be monitored to infer the strength of titan ' s winds , and the huygens atmospheric structure instrument ( hasi ) will measure temperature , pressure and electrical fields that could indicate the presence of lightning 下降过程中将持续监测探测器无线电讯号的频移，以推算土卫六风场强度；而惠更斯大气结构仪（ hasi ）会量测温度、气压以及可能显示闪电是否存在的电场。
	6.	One of the interesting properties of infra - sound is that it can travel a long distance in the air without much decay . this enables continuous monitoring of the atmosphere on a large scale . when combined with other remote sensing data , it can provide additional information regarding the atmospheric structure 次声波的特点是衰减小，可作长距离传播，因此能够对大气进行大范围连续不断的监察，当结合其他的遥感资料一起使用，更可提供额外的关于大气结构的数据。
	7.	An atmosphere structure constant cn2 model , which varies with height , is presented based on itu - r amplitude scintillation model , existing itu - r optical cn2 model and meteorologic measurement relative humidity and temperature profile data , at 10 ~ 30ghz . the log - amplitude scintillation deviation calculated in terms of the cn2 model based on humidity and temperature vertical profile compare with values predicted by means of itu - r and ortgies model . it is emerged that the calculation results based on the cn2 model agree almost with prediction results by itu - r and ortgies model at 10 ~ 30ghz and there is an advantage that relative humidity and temperature varied with height has be considered in the cn2 model 根据光波段的itu - rc _ n ~ 2模型， itu - r幅度闪烁标准偏差模型，和温度和相对湿度随高度变化的气象数据，在10 30ghz ，分析得到了大气结构常数c _ n ~ 2随高度变化的模型；并根据温度和湿度垂直分布数据计算了对数幅度闪烁_ x ，还与itu - r和ortgies模型的预测结果进行了比较，结果表明，在10 30ghz ，用该c _ n ~ 2模型计算的结果和用itu - r及ortgies模型预测的值符合较好，且在用c _ n ~ 2模型计算时考虑了温度和相对湿度随高度变化关系。
	8.	According to the theory of optical wave propagation in the slant path and the itu - r turbulence structure constant model , which is altitude dependent and proposed in 2001 , the modified rytov method is extended to be applied to study on the problems , which waves propagate in the slant path . the scintillation index as a function of the rytov variance is obtained from weak to strong fluctuation regions with plane wave and sphere wave incidence , respectively 根据斜程传输理论和2001年提出的itu - r湍流大气结构常数模型，将修正pytov方法推广应用于斜程传输问题研究，得到了平面波和球面波斜程传输时的闪烁指数，分析了湍流内尺度、近地面风速等参量对闪烁指数的影响。
	9.	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。

Similar Words：

"大气降水中氟化物的测定" Chinese translation, "大气降水中硫酸盐测定" Chinese translation, "大气降水中氯化物的测定" Chinese translation, "大气降水中硝酸盐测定" Chinese translation, "大气降水中铵盐的测定" Chinese translation, "大气结构切面纹" Chinese translation, "大气结构研究卫星" Chinese translation, "大气界面" Chinese translation, "大气斤射" Chinese translation, "大气进气歧管绝对压力" Chinese translation