「interferometry」の共起表現(1語右で並び替え)

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「interferometry」の共起表現一覧(1語右で並び替え)

interferometry

1語右で並び替え

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Electronic Speckle Pattern Interferometry, also known as TV holography, uses video d
Dual Polarisation Interferometry, an analytical technique used to measure t
ntrol algorithms for long-baseline optical interferometry; analytical and numerical techniques for t
of the available antennas Pawsey used sea interferometry and began observations at Dover Heights wh
cosmology and all aspects of astronomical interferometry, and operating the Mullard Radio Astronomy
is is a unique characteristic of bio-layer interferometry and extends its capability to perform in c
profilers, ellipsometry, dual polarisation interferometry and scanning electron microscopy of cross-
uorescence spectroscopy, dual polarisation interferometry and computational methods, coupled with th
rements, from Hipparcos and Tycho, speckle interferometry, and other sources.
onabarabran), to form a very long baseline interferometry array.
geodetic and astronomic very long baseline interferometry as a member of the European VLBI Network.
ts that photon-entanglement, combined with interferometry, can possibly be used to remote-sense dist
al processing technique of beamforming and interferometry can be used to calculate the distance and
ce plasmon resonance and dual polarisation interferometry can also quantify the affinity from concen
erferometers and a History of astronomical interferometry can be referenced from their respective pa
ching surface plasmon resonance, Bio-Layer Interferometry, Coimmunopreciptation indirect ELIS, equil
asure the angular diameter of a star using interferometry, converting the 80 cm telescope at Marseil
imental techniques using Vertical Scanning Interferometry, Electron and Atomic Force Microscopy and
Seismic interferometry essentially exploits the phase difference
ferent analysis such as SAR, polarization, Interferometry etc.
tor instrument, while DASI is a famous CMB interferometry experiment credited with the first detecti
in the first successful very long baseline interferometry experiment in the 1960s.
terferometer, constructed after successful interferometry experiments using the pre-existing 15-metr
d optical gating (FROG), or Spectral phase interferometry for direct electric-field reconstruction (
Spectral phase interferometry for direct electric-field reconstruction (
DER is an implementation of Spectral phase interferometry for direct electric-field reconstruction (
PIDER) is an advancement of Spectral phase interferometry for direct electric-field reconstruction (
glacier surge measured by satellite radar interferometry, Geophysical Research Letters, 29(23), 209
In optical interferometry, homodyne signifies that the reference rad
gh it was observed to be binary by speckle interferometry in 1985, subsequent observations show no s
ne of the ε2 pair, was detected by speckle interferometry in 1985 and confirmed in two subsequent ob
With the advances in optical interferometry in the 1990s, Schedar's angular diameter w
Interferometry inherently depends on the wave nature of t
Dual polarisation interferometry is a quantitative analytical method for me
Dual polarisation interferometry is an optical technique which can measure
Interferometry is the process of combining waves in such
Bio-Layer Interferometry is a label-free technology for measuring b
Dual Polarization Interferometry is used to quantify the order and disrupti
Laser-based interferometry is often used for air flow measurement, bu
Self-mixing interferometry is a measurement technique, in which a las
r this is that in all these techniques the interferometry is used to linearize detection transfer fu
ptical instrument design, aspheric optics, interferometry, lasers, and lens testing, Hopkins has bee
NASA's planned Space Interferometry Mission (SIM PlanetQuest) will utilize ast
project scientist for the NASA/JPL "Space Interferometry Mission" to search for Earth-like exo-sola
So in next decade, the Gaia mission, Space Interferometry Mission, or James Webb Space Telescope wil
arcsecond to the early stages of the Space Interferometry Mission.
Radar and speckle interferometry observations show that the shape of Victor
at lower resolution using Aperture Masking Interferometry on the William Herschel Telescope).
The technique is also known as feedback interferometry or induced-modulation interferometry.
dy of the system by long-baseline infrared interferometry performed at Palomar Observatory found no
Seismic interferometry provides for the possibility of reconstruc
White-light interferometry scanning (WLS) systems capture intensity d
mates of the level of holographic noise in interferometry show that it must be much smaller in magni
Radio interferometry started in the mid-1940s on the outskirts
ion-absorption infrared, dual polarisation interferometry, surface enhanced Raman, and sum frequency
Using such an interferometry technique can provide certain geometric la
luate the plasma densities by the means of interferometry techniques.
optical setups, especially those involving interferometry, the alignment of each component must be e
oscopy, ellipsometry, or dual polarisation interferometry, the QCM determines the mass of the adsorb
In immersion Mirau interferometry, the interference patterns needed to repro
de electric and magnetic probes, microwave interferometry, Thomson scattering and charge exchange sp
ravitational wave detector that uses laser interferometry to detect the influence of gravitational w
measure gravitational waves by using laser interferometry to monitor the fluctuations in the relativ
Both of these experiments used radio interferometry to measure CMB fluctuations at lower resol
There, from 1932-34 he researched interferometry under Prof. A. Fowler and began writing "H
A special application of optical interferometry using coherent light is Holographic interf
f the spectral line emitted by krypton-86, interferometry was essential in setting up the standard.
In the 1940s radio interferometry was used to perform the first high resolut
l imaging technique based on low-coherence interferometry, where subsurface light reflections are re
red positions, allowing aperture synthesis interferometry with a maximum baseline of 36 km (22.3 mil
An extensive review article "Optics and interferometry with atoms and molecules" appeared in July
star has been measured using long baseline interferometry, yielding a value of 9.09 ± 0.09 milliarcs