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Home > english-chinese > "atmospheric structure" in Chinese

Chinese translation for "atmospheric structure"

大气结构

Related Translations:
atmospheric sciences:  大气科学大气学
atmospheric vortex:  大气涡流大气涡旋
atmospheric turblence:  大气湍流
atmospheric scientist:  大气科学家
atmospheric electricity:  大气电学;大气电天电,大气电
atmospheric exploration:  大气探测
atmospheric dinamics:  大气动力学
atmospheric constituent:  大气组分;大气组元大气组元
atmospheric recovery:  在大气层回收
atmospheric inversion:  大气逆变;大气逆温大气逆温
Example Sentences:
1.Studies of jupiter ' s atmospheric structure and storm behavior
研究木星的大气层结构与天气系统
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.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。
4.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。
5.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:
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