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Перевод: interferometer

[существительное]
интерферометр

Тезаурус:

1. However, the time that the light remains inside the interferometer arms is then, which means that the measurement time must be equally long or longer.
2. Furthermore, we have made very-long-baseline interferometer (VLBI) observations of the main features and of the strongest redshifted feature at v LSR =1,322 kms -1 , by using the 45-m and the Kashima 34-m telescopes.
3. A preferred method for detecting the relative movement is to build a Michelson interferometer with the mirrors mounted on these freely suspended blocks.
4. An interferometer swung around by the Earth's rotation will "synthesise" a dish as large as the separation of the two telescopes.
5. LEFT A fixed radio interferometer aerial, 440 m long, at the Mullard Radio Astronomy observatory, Cambridge, England.
6. It is worth noting that, although an interferometer can in principle respond to any frequency, the bandwidth is restricted in practice by the photon storage time to .
7. With one of the pair in orbit, the interferometer swings around much more rapidly - reducing the time required for observing each source - and the separation is not limited by the size of the Earth: present technology permits a radio telescope in an orbit a hundred times larger, improving the resolution a hundredfold over that possible from Earth
8. These cheap, reliable and effective instruments have now been challenged by the alternative type, the interferometer.
9. One variety uses a freely suspended massive bar cooled to 4 K and another variety uses a large Michelson interferometer monitored with laser beams.
10. Figure 10.5 shows a plan view of a large Michelson interferometer in which the three blocks carrying the mirrors M, M 1 , and M 2 are freely suspended.
11. The two bodies labelled A and B in Fig. 2.3 carry corner cube mirrors C A A and C B while B also carried a beam splitter S. These optical components are used as elements of a Michelson interferometer; the source is a stabilized He-Ne laser and the detector is a p-i-n photodiode.
12. Radio telescopes on the Earth have a resolution limited by their size, or, in the case of a pair of telescopes linked as an interferometer, by their separation.
13. Such motion should be detectable either from timing measurements, or from relative astrometry with the Parkes-Tidbinbilla Interferometer or with Parkes-Hobart very-long-baseline interferometry.