「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)

interferometer

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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