Sentence examples for mm wavelength from inspiring English sources

Sensors technologies of all kinds such as electro-optics, acoustic, active/passive UV to LWIR, ground-penetrating radar, passive mm wavelength, X-ray tomography, neutron activation imaging, multi-spectral, hyper-spectral, and ultra-spectral imaging, will provide valuable images that normal CCD camera cannot offer.

A portable instrument has been developed with which it is possible to measure longitudinal railhead irregularities to an accuracy of about 1 micron r.m.s. in the 30 100 mm wavelength range, with slightly poorer accuracies in shorter and longer wavelength ranges.

In the present study, titanium diboride of submicron sizes were incorporated to the titanium substrate by a selective laser melting (SLM) process of Ti + (10, 15 or 20 vol%) TiB2 powder mixtures via an Ytterbium fiber laser with 1.075 mm wavelength.

In contrast to that, Berner and Evenari (1978) measured only 0.005% of the incident light at a depth of 10 mm, Schlesinger et al. (2003) observed 2.8% of the incident light at a depth of 12 mm (wavelength: 680 nm), and Broady (1981) found that 2.7% of the incident light reached the bottom of a 13 mm thick stone.

The visual display on a horizontal table consisted of circular LEDs (each LED on 2.9 mm, wavelength 636 nm with intensity of luminous 60 mcd) placed at two viewing distance in middle line, one at 20 cm from the subject, and the other at 150 cm.

Bolometer, designed to detect incident power, is a popular instruments in space radiometry, for sub-mm wavelength observations and thermal imaging for military and biomedical applications.

These results thus demonstrate that mm-wavelength radiation can be coupled to CO molecules located at less than 50 µm above the surface of the chip a few hundredths of the wavelength and rotational spectra were obtained with a resolution of approximately half a MHz.

It detects light at "sub-mm" wavelengths.

The normal metal hot-electron microbolometer (NHEB) is a direct detector for mm and sub-mm wavelengths.

The apex-sz instrument is designed for the discovery and study of galaxy clusters at mm-wavelengths using the Sunyaev Zel'dovich effect.

We focus on recent experiments which have mapped the sky at mm/sub-mm wavelengths, improving our knowledge of the Galaxy and of the Cosmic Microwave Background (CMB), and on near future experiments directly derived from these.