What is the translation of " INTERFEROMETRY " in Chinese?

• 干涉测量
• 干涉

Examples of using Interferometry in English and their translations into Chinese

Previem Interferometry.
端面预览+干涉测量.

Indeed, CHIRP could be applied to any imaging system that uses radio interferometry.
CHIRP还可用于任何使用无线电干涉测量的成像系统。

The Laser Interferometry Space Antenna.
激光干涉空间天线.

Adequate preparation of the specimen is essential in order to obtain the highest precision in multiple-beam interferometry.
试样充分的准备是必不可少的，以获得最高的精度在多光束干涉。

Radar interferometry techniques were appropriate for mountain areas.
雷达干涉测量技术适合在山区使用。

It was also to test space-based interferometry with Longjiang-1.
还用龙江-1测试了基于空间的干涉测量法。

In optical interferometry, this reference plate is known as the reference plate(or reference mirror).
在光学干涉测量，该参考平面被称为基准板（或参考反射镜）。

It has been resolved using speckle interferometry at a distance of 0.25" in 1972.
在1972年用散斑干涉解析出它的距离为0.25"。

Differential interferometry techniques were also useful for measuring millimetric displacements in the terrain.
差动干涉测量技术在测量地形以毫米计的位移方面也非常有用。

However, this can, in fact, be accomplished by two-beam interferometry even without a phase contrast microscope.
然而，这可以，实际上，可以通过双光束干涉，即使没有相位差显微镜来完成。

His research interests include optical spectroscopy for early cancer detection, novel microscopy and interferometry techniques.
他的研究兴趣包括用于早期癌症检测的光谱学，新型显微镜学和干涉测量技术。

RadioAstron Very-Long Baseline Interferometry instrument: project in hibernation.
射电天文甚长基线干涉测量仪器：项目搁置.

Atom interferometry, however, hinges on quantum mechanics, the theory that describes how matter behaves at sub-microscopic scales.
然而，原子干涉测量法取决于量子力学，这种理论描述了物质在亚微观尺度上的表现。

Radioastron very-long-base interferometry instrument: project in hibernation.
射电天文甚长基线干涉测量仪器：项目处于搁置状态.

The contrast displayed by minute level changes can be enhanced to an even greater extent than is possible when utilizing two-beam interferometry.
分钟级别变化的对比显示，可以更大程度的提高，可能比时，利用双光束干涉。

It is widely used in microscopes, imaging and fields like interferometry, industry, life sciences, testing and measurement.
它广泛用于显微镜，成像和干涉测量，工业，生命科学，测试和测量领域。

Very long baseline interferometry, or VLBI, is a technique that combines waveforms recorded by two or more radio telescopes.
极长的基线干涉测量法或VLBI是一种组合由两个或多个射电望远镜记录的波形的技术。

The fine-resolution mode, a strip SAR, is a conventional mode, used mainly for detailed regional observations and repeat-pass interferometry.
精确分辨率形式，即条幅式合成孔径雷达是一种常规形式，主要用于详细的区域观测和干涉测量中继扫描。

A technique called radar interferometry is also used in the study to process high-resolution data and reveal surface changes.
研究中还用到名为“雷达干涉测量”的技术，可以处理高分辨率数据并揭示地表变化。

Initiation of monitoring work on hydraulic structures using satellite-based global positioning systems(GPS) and radar interferometry technologies;
启动关于利用全球卫星定位系统（GPS）以及雷达干涉测量技术对水文结构进行监测的工作。

The two detection techniques(B-modes and laser interferometry) are searching for waves at different frequencies- 15 orders of magnitude apart.
两种检测技术(B模和激光干涉)正以不同频率寻找引力波--相差15个数量级。

The above elements would be addressed by implementing three separate data-processing chains: change detection; microclimate; and interferometry integrated into a geographic information system.
上述因素将通过实施三个独立的数据处理链来处理：变化探测；微气候；以及纳入地理信息系统的干涉测量。

Methods such as X-rays and lasers or white light interferometry demand precise positioning of the specimens to be examined and of optics or beam control.
X射线和激光以及白光干涉测量等方法都需要精准定位待测样本及精准的光学元件或光束控制。

Since the laser interferometry gravitational wave observatory(LIGO) was launched in 2015, scientists have had the technology to measure gravitational waves.
自2015年激光干涉引力波天文台（LIGO）上线以来，科学家便拥有了测量引力波的技术。

Such arrays would be capable of achieving high-resolution astronomy and interferometry at lower costs, and could free up large, complex arrays for other observations.
这种阵列能够以较低的成本实现高分辨率的天文学和干涉测量，并且可以释放大型复杂阵列用于其他观测。

Consequently, in any type of interferometry, the continuity of the fringes should first be ascertained with white light in order to avoid substantial errors.
因此，在任何类型的干涉，这些条纹的连续性应先用白色光，以避免实质性的错误确定。

These observatories combine their data using very-long-baseline interferometry to create a virtual telescope that has an effective diameter of the entire planet!
这些天文台使用非常长的基线干涉测量法将他们的数据结合起来，创造出一个有效直径等于地球的虚拟望远镜!