脉泽的英文

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"脉泽"怎么读用"脉泽"造句

英文翻译手机版

[物理学] (微波激射器; 受激辐射微波放大器) maser (microwave amplification by stimulated emission of radiation)

"脉"英文翻译 affectionately; amorously; l ...
"泽"英文翻译 pool; pond
"声脉泽" 英文翻译 : acoustic maser
"半导体脉泽" 英文翻译 : semiconductor maser
"共振腔脉泽" 英文翻译 : cavity maser
"固态脉泽" 英文翻译 : solid state maser
"光量子脉泽" 英文翻译 : light quantum maser
"晶体脉泽" 英文翻译 : crystal maser
"空腔脉泽" 英文翻译 : cavity maser
"冷却式脉泽" 英文翻译 : cooled maser
"脉泽发射机" 英文翻译 : maser transmitter
"脉泽放大" 英文翻译 : maser amplification
"脉泽放大器" 英文翻译 : maser amplifier
"脉泽辐射" 英文翻译 : maser radiation
"脉泽跃迁" 英文翻译 : maser transition
"脉泽振荡器" 英文翻译 : maser oscillator
"气体脉泽" 英文翻译 : gasmaser
"三脉泽兰油" 英文翻译 : ayapana oil
"三能级脉泽" 英文翻译 : three level maser; three-level maser
"射束脉泽" 英文翻译 : beam type maser
"深水光脉泽" 英文翻译 : deep-sea optical maser
"双能级脉泽" 英文翻译 : two level maser
"天体脉泽" 英文翻译 : astronomical maser; astrophysical maser
"天体脉泽源" 英文翻译 : celestialmaser
"天文脉泽" 英文翻译 : astronomical maser; astrophysical maser

例句与用法

A new generating mechanism for interstellar oh and their masers
及其脉泽的一种新的发生机制
Influence of chloroform on the ir spectra of aromatic amines
脉泽源在银河系中的分布和空间运动
Besides acting as powerful signposts of active star formation , the intense maser emission provides a unique tool to probe the physical conditions and kinematics of these regions on scales of 10 - 103 au
星际脉泽不仅是恒星形成的一个及其重要的标志，而且也提供围绕大质量恒星尺度10 - 10 ~ 3au分子气体的物理条件和动力学结构的信息。
To understand the connections between methanol masers and other phenomena typical of star formation region , such as the associated far - infrared sources , we have investigated statistical properties of all known 6 , 7 ghz methanol maser sources . the result suggests that 6 , 7 ghz methanol maser emission may appear only during a limited period of massive star formation
6 . 7ghz甲醇脉泽源的统计结果暗示着它们可能仅仅发生在大质量恒星形成的一个很短的时段内，可能起源于拱核盘中或外流中，远红外辐射则是一种可能的抽运机制。
To search for high - velocity molecular emission toward massive star formation regions , and to study the connections between h2o masers , iras objects and outflow properties , we carried out a co observation for a h2o maser sample . we found that most of the objects have excess high velocity emission produced by outflows ; we find a significant correlation between co line full widths and iras luminosities . the widths are proportional to the iras luminosities
通过在大质量恒星形成区搜寻高速分子辐射，并且研究它们与星际h _ 2o脉泽源和所联系的红外源之间的关系，我们发现绝大多数源都存在着气体的高速运动并且它们是由分子外流产生的；我们同时发现在co分子的谱线全宽和所对应源的红外光度之间存在很好的相关性，线宽随红外光度增加而变大。
From some characteristics observed , such as the short lift time , narrow frequency band , fast frequency drift , quasi - periodic pulsation , spike event and complex magnetic structure , it is considered that the radiation mechanism of these events may be principally due to the electromagnetic waves magnified directly by the instable electronic cyclotron
从它们的观测特征：短寿命，窄频带，频率快速漂移，及尖峰事件与磁结构复杂的大黑子活动区密切相关等，认为这些事件的辐射机制可能是电子回旋脉泽不稳定直接放大电磁波所致。
In order to better understand the excited mechanism of masers , we have studied the time variability of 22 ghz h2o masers in ggd25 , an outburst with the time scales of 4 day was detected . the time variation was probably caused by a collsion pump which led to changes in the pump input
为了更好地理解脉泽的产生机制以及脉泽和恒星形成区的一些典型现象，如它们所联系的远红外源之间的关系，我们研究了22ghzh _ 2o脉泽源的时变以及所有已知的6 . 7ghz甲醇脉泽源的统计性质。