「interferometer」の共起表現(1語右で並び替え)

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「interferometer」の共起表現一覧(1語右で並び替え)

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The Jamin	interferometer allows very exact measurements of the refr
ptics system, a coronagraph, a calibration	interferometer, and an integral field spectrograph.
oduce 100 fringe cycles in the measurement	interferometer and 50 in the reference interferometer.
Start with a Mach-Zehnder	interferometer and a light source which emits single phot
The Michelson	interferometer and Mach-Zehnder interferometers are examp
tical interleaver: 1) Step-phase Michelson	interferometer, and 2) Birefringent crystal networks.
precursors of Minitrack are evident in the	interferometer arrangement.
omic clocks was recognized also as an atom	interferometer at the PTB in Braunschweig, Germany.
nterferometrically by the Mark III Stellar	Interferometer at Mount Wilson Observatory, California, U
the decommissioning of the MISTRAM X-band	interferometer at the Air Force Eastern Test Range in 197
observations were made with the Cambridge	Interferometer, at 81.5 MHz.
VIRGO is a 3 kilometer	interferometer built through a French-Italian collaborati
The first such	interferometer built was at the Mount Wilson observatory,
was based on an earlier optical intensity	interferometer built by Hanbury Brown and Richard Q. Twis
The 3C survey also used the Cambridge	Interferometer, but at 159 MHz, which helped significantl
The former is based on Michelson	interferometer combined with Gires-Tournois interferomete
d space mission to build a double-aperture	interferometer composed of three free-flying satellites.
The	interferometer consisted of an array of 4 fixed elements
yama Millimetre Array (NMA): An millimetre	interferometer consisting of six 10m diameter telescopes.
The	interferometer consists of a long plate of glass or quart
t is the first purpose-built submillimeter	interferometer, constructed after successful interferomet
ation-isolation system, a suspension point	interferometer, cryogenic mirrors, a resonant side band e
214 MHz using the 2-element Long Michelson	Interferometer), discovering some of the most interesting
An	interferometer does not detect light in quite the same wa
A search with a near-infrared speckle	interferometer failed to detect a companion orbiting 1-10
isotropy Telescope CAT was a three-element	interferometer for cosmic microwave background radiation
	Interferometer for measuring the interference properties
Figure 3: Fizeau	interferometer for measuring the effect of water movement
) diameter radio telescopes arranged as an	interferometer for submillimeter wavelength observations.
The CHARA Array is an	interferometer formed from six 1 meter (40-inch) telescop
The DECi-Hertz	Interferometer Gravitational wave Observatory (or DECIGO)
(The	interferometer had previously been used for the 2C survey
The air-wedge	interferometer has a very simple design and requiring onl
I began operation in 1964 as a two element	interferometer in order to test large aperture synthesis
One simple layout of an astronomical	interferometer is a parabolic arrangement of mirrors, giv
ach distance to be measured, a measurement	interferometer is built using optical components placed a
An X-ray	interferometer is analogous to a neutron interferometer.
The Jamin	interferometer is a type of interferometer, related to th
The N-slit	interferometer is an extension of the double-slit interfe
The setup of the Twyman-Green	interferometer is similar to that of the Michelson interf
A point diffraction	interferometer is a type of common path interferometer.
The length of each measurement	interferometer is given in units of reference length by t
A Twyman-Green	interferometer is a variant of the Michelson interferomet
The measured	interferometer is therefore twice the length of reference
In a WLS system, an imaging	interferometer is vertically scanned to vary the optical
First, the fixed mirror in the Michelson	interferometer is rotatable in the Twyman-Green interfero
The Michelson stellar	interferometer is one of the earliest astronomical interf
The	interferometer is made up of two mirrors, made of the thi
The reference arm of a Mirau	interferometer is located within a microscope objective a
The interference on a Sagnac	interferometer is proportional to the enclosed area.
An	interferometer is an optical measuring device using the p
An acoustic	interferometer is an instrument for measuring the physica
The optical path of each measurement	interferometer is compared to the optical path in a refer
A Michelson	interferometer makes use of a separate light source and d
The	interferometer measures resonant frequency of the cantile
rwin Mission and Terrestrial Planet Finder	interferometer missions, and would involve many large fre
A 20-foot (~6 meters) Michelson	interferometer mounted on the frame of the 100-inch (~250
rvations of 51 Ophiuchi made with the Keck	Interferometer Nuller at the W. M. Keck Observatory show
CLIO is the Cryogenic Laser	Interferometer Observatory, a prototype detector for grav
The ring	interferometer of the Michelson-Gale experiment was not c
catalogue was produced using the Cambridge	Interferometer on the west side of Cambridge.
The CHARA Array is an optical astronomical	interferometer operated by The Center for High Angular Re
of Tenerife, and the Degree Angular Scale	Interferometer, operated in Antarctica.
It was a 13-element	interferometer operating between 26 and 36 GHz in ten ban
d optical intensity maxima or minima of an	interferometer or diffractive optical element.
The Lummer-Gehrcke	interferometer or Lummer-Gehrcke plate is a multiple-beam
Background Imager (or CBI) is a 13-element	interferometer perched at an elevation of 5,080 metres (1
hysical property that makes the ring laser	interferometer process a self-calibrating process.
uent statistical analysis by Hewish of the	interferometer records later showed some aspects of the i
The first modern atom	interferometer reported was a Young double slit experimen
A study with the Palomar Testbed	Interferometer revealed that Altair is not spherical, but
ubly modulated, both by the PEM and by the	interferometer setup.
etition from two other missions, the Laser	Interferometer Space Antenna (LISA) and the International
trong enough to be detected with the Laser	Interferometer Space Antenna.
ne gravitational wave detector LISA (Laser	Interferometer Space Antenna), and he was instrumental in
Laser	Interferometer Space Antenna (LISA) (2015): a gravitation
(BBO) is a proposed successor to the Laser	Interferometer Space Antenna (LISA).
Constellation-X and the Laser	Interferometer Space Antenna (LISA) been promoted by NASA
ence of light requires a nonlinear optical	interferometer, such as an intensity optical correlator,
Although an amplitude splitting	interferometer such as the Michelson interferometer could
Unlike an amplitude splitting	interferometer, such as a Michelson, which separates out
d's only long-baseline (437-meter) optical	interferometer that can simultaneously co-phase six eleme
As in a Fabry-Perot	interferometer, the light that leaks out has phase that d
riments including the Degree Angular Scale	Interferometer, the Sunyaev-Zel'dovich Array, and the Sou
val Observatory later constructed a larger	interferometer, the Navy Prototype Optical Interferometer
hifting element is added to one arm of the	interferometer, then the displacement it causes can be de
COAST was the first long-baseline	interferometer to obtain high-resolution images of the su
several weaker sources in the lobes of the	interferometer to produce the apparent effect of a single
very important when coupling the air-wedge	interferometer to imaging optics.
, will turn the lateral-shearing air-wedge	interferometer to a radial-shearing interferometer, which
Fiber optic current sensor, using an	interferometer to measure the phase change in the light p
e, the disk around 51 Ophiuchi requires an	interferometer to resolve, in contrast to that of Beta Pi
Development of both the passive	interferometer type of FOG, or IFOG, and a newer concept,
An image of the	interferometer used in the core of the Planetary Fourier
on of the Michelson-Morley experiment, the	interferometer used starlight as the source of light.
ine if such a fringe shift took place, the	interferometer was made extremely stable and the interfer
its extremely thin air-gap, the air-wedge	interferometer was successfully applied in experiments wi
The Mark III Stellar	Interferometer was a long-baseline astronomical optical i
From 1980-1985 a 3-element	interferometer was constructed, with another four antenna
The	interferometer was proposed by Albert Michelson in 1890,
The Cambridge	Interferometer was a radio telescope interferometer built
The Mark III	interferometer was used to resolve a number of spectrosco
ite starting in the 1970s when a 2-element	interferometer was constructed.
The GMRT is an	interferometer which uses a technique known as aperture s
s heated by the powerful laser used in the	interferometer) while keeping them isolated from vibratio
ce, a power supply, a control unit, and an	interferometer with electronics.
elescope", an extremely large astronomical	interferometer with spherical geometry that might theoret
e, is a multi-element optical astronomical	interferometer with baselines of up to 100 metres, which
It is an optical	interferometer with two perpendicular arms 1000 m long.
ly 1950s when the Navy picked up the Azusa	interferometer work for its Viking project at White Sands
A Mirau	interferometer works on the same basic principle as a Mic

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「interferometer」の共起表現一覧(1語右で並び替え)