「Wavelength」の共起表現(1語右で並び替え)

Weblio 辞書 > 英和辞典・和英辞典 > Wavelengthの意味・解説 > Wavelengthに関連した共起表現

意味

例文

類語

共起表現

「Wavelength」の共起表現一覧(1語右で並び替え)

該当件数 : 322件

1 2 次へ＞

nfrared detectors, each sensing a particular	wavelength, a temperature profile, or sounding of the a
	Wavelength ABC, a children's opera
It may be used to measure velocity,	wavelength, absorption, or impedance.
pulsed lasers, time domain optimized lasers,	wavelength adapted lasers, and ultra compact modular la
esents refractive index, the "D" denotes the	wavelength, and the 20 denotes the reference temperatur
ossible lattice vibration has a well-defined	wavelength and frequency.
tage of fluorospheres is that the excitation	wavelength and the emission wavelength are not the same
hear distance, df the fringe distance, λ the	wavelength and γ the angular deviation of the fringe al
It operates at 81.5 MHz (3.7 m	wavelength), and is made up of 4096 dipoles in a phased
The detectors were designed to measure	wavelength and flux shifts of solar radiation during pe
otoluminescence at room temperature, and its	wavelength and lifetime can be tuned by substitution of
This laser has high beam uniformity, short	wavelength, and the ability to modify the spot size to
xpressed in wavenumber, λ0 is the excitation	wavelength, and λ1 is the Raman spectrum wavelength.
ty of tunable laser light at the appropriate	wavelength and also the availability of high reflectanc
Because of their	wavelength and precision, CO2 lasers remain the dominan
Single	wavelength anomalous dispersion (SAD)
esults, the antennas should be spaced half a	wavelength apart, or less.
r is identical, or is one (or other integer)	wavelength apart.
Light of this	wavelength appears capable of increasing activity of cy
surrounds the galaxies absorbs light with a	wavelength around 100 nanometers, the galaxies have a n
The Long	Wavelength Array (LWA) is a radio telescope under const
photons have the same energy (frequency) and	wavelength as the incident photons.
RWA (Routing	Wavelength Assignment) in Optical Burst Switching of Op
how a drop in the continuum radiation at the	wavelength associated with the absorbed photons.
To get a single and fixed	wavelength at the end station, a monochromator is used.
Monochromators have one exit slit and one	wavelength at a time can pass through that slit.
a black hole is roughly equal to the Compton	wavelength at the Planck scale, a photon with sufficien
'capacity hat', which extends the electrical	wavelength, at the top.
45, 14.9 and 32.5 GHz (i.e. 3, 2 and 1 cm in	wavelength) at the Teide Observatory, Tenerife.
than λ0, M(λ) is negative and increases with	wavelength; at wavelengths longer than λ0, M(λ) is posi
em of the chromophore, they may increase the	wavelength at which the light is absorbed and as a resu
pler has four ports, each placed one quarter	wavelength away from each other around the top half of
this general shape are absorption features (	wavelength bands where the intensity is lowered) that h
be recorded sequentially at different narrow	wavelength bands.
After 20 years of the 104.9	wavelength being based at Regent House, Stockport, Imag
eed, oxygen gas absorbs the radiation with a	wavelength below 195 nm.
Fused quartz, with a	wavelength below 380 nm (ultraviolet spectrum)
(FSR) is the spacing in optical frequency or	wavelength between two successive reflected or transmit
W0 is defined as the difference in	wavelength between the points on either side of the emi
web camera can be used for video detection (	wavelength between 0.4 and 0.7 µm).
r systems are differentiated not only by the	wavelength, but also by the light delivery system: flex
hould not only absorb laser light of a given	wavelength, but they should also be able to withstand a
The emission	wavelength can be lowered by substituting the anthracen
es the frequency between 5600-5650 MHz (5 cm	wavelength) carrier wave, with an angular resolution be
The reflected	wavelength changes with the grating period, broadening
elocity of the wave remains constant whereas	wavelength changes; hence frequency also changes.
offset by the extra distance that the longer	wavelength components have to travel through the second
for the discrimination of light based on its	wavelength components.
tion) the remaining power at longer infrared	wavelength contained basically two components: the CIB
However, as shorter	wavelength continuous spectrum "X-ray" sources such as
ptical switching, electro-optical switching,	wavelength conversion, reconfigurable optical delay lin
l, Plymouth Evening Herald, The West Briton,	Wavelength, Cornwall Today magazine, Brides in Cornwall
Where λg is the	wavelength corresponding to the central rejection frequ
ptical telecommunications, allowing all-band	wavelength coverage and in-line distributed signal ampl
-rich areas of the sky in terms of depth and	wavelength coverage.
the optical rotation first increases as the	wavelength decreases (as first observed by Cotton), and
se to familiar absorption of light, which is	wavelength dependent and gives rise to colours.
The flux of light is not very	wavelength dependent because the cloud droplets are lar
or one instrument both energy dispersive and	wavelength dispersive instrumentation is available prov
The	Wavelength dispersive X-ray spectroscopy (WDXRF or WDS)
ws to use an intense beam of neutrons with a	wavelength distribution of 10% or more and at the same
arameters of fluorescence: its intensity and	wavelength distribution of emission spectrum after exci
However, when used in	wavelength division multiplexing systems, dispersion-sh
tle therapeutic approach is dependent on the	wavelength, dosage, pulsation, and intensity being appl
very organism's bioluminescence is unique in	wavelength, duration, timing and regularity of flashes.
delay time of the acceleration power, laser	wavelength, energy density of the laser and the impact
parameters (dose, type of laser, materials,	wavelength, etc.) have not been identified.
where λ is the	wavelength, f is the frequency, and c is the speed of p
Both series' were produced by	Wavelength Films for ITV London, and series one was als
53 cm (553 to 566 MHz) - an extremely short	wavelength for the time - with a pulse length of 2 micr
er which the 'operator' had to listen on the	wavelength for three minutes for possible instructions
oscopy, however it can operate with only one	wavelength for excitation and depletion.
capture data in 36 spectral bands ranging in	wavelength from 0.4 µm to 14.4 µm and at varying spatia
Glass, with a	wavelength from 380 to 780 nm (visible spectrum)
Plastic, with a	wavelength from 380 to 780 nm (visible spectrum)
rofile tailored to shift the zero-dispersion	wavelength from the natural 1300 nm in silica-glass fib
version, the S-band (2500-3700 MHz, 12-9 cm	wavelength) FuMB7 Naxos U, was provided to U-boats to a
Small changes of the incident	wavelength generated by an acousto-optic modulator or i
ive index yields selective reflection of the	wavelength given by the helical pitch, allowing the liq
ss operated at a frequency of 85.5 MHz (3.5m	wavelength), giving a 49 arcminute beam.
aphy to monitor small deformations in single	wavelength implementations as well as dimensional metro
The	wavelength in this band varies from one to one tenth of
fields within astronomy, using wide range of	wavelength in observation.
imensions that are large with respect to the	wavelength in question but small with respect to the be
ily cascaded, thus accessing essentially any	wavelength in the fiber low-loss guiding windows (both
The horizontal axis is	wavelength in nm.
e telescope is intended to observe in longer	wavelength infrared than the James Webb Space Telescope
ission from a blackbody that is in a certain	wavelength interval or band.
rce wavelengths are λ1 and λ2, the resulting	wavelength is
Because the 15-meter	wavelength is harmonically related to that of the 40-me
n exists when the ratio of the period to the	wavelength is near one; in this case, a holographic gra
half-wavelength past the load; this flexural	wavelength is determined in large part by the elastic t
ed after each slit so that the light at each	wavelength is measured by a different detector.
n be transferred by an optical fiber, as its	wavelength is not absorbed much by fused silica but is
the anomalous dispersion that occurs when a	wavelength is selected that is in the vicinity of an ab
The	wavelength is often selected to be the one at which the
Each infrared	wavelength is sensitive to temperature and water vapor
adiations, in which a photon of a particular	wavelength is absorbed and an equivalent photon is imme
When light of the appropriate	wavelength is coupled to the loop by the input waveguid
o that of an ideal Gaussian beam at the same	wavelength is denoted M² ("M squared").
This	wavelength is absorbed by the atmosphere, effectively a
Since	wavelength is often expressed in units of nanometers (n
orescence microscopy in which the excitation	wavelength is shorter than the emission wavelength, as
Additionally, the peak emission	wavelength is about 480 nm.
frequency of a standing wave where a quarter	wavelength is the distance between the base of the mug
produce a diffraction pattern because their	wavelength is typically the same order of magnitude (0.
This dependence of specific rotation on	wavelength is called optical rotatory dispersion.
But when activated by light of a certain	wavelength, it has a major impact on the cornea," NBC's
It absorbs far-red light, at 710 nm	wavelength, just outside the optical range.
microseconds, de-excite and emit light at a	wavelength larger than the excitation wavelength.
TD 110 Dual	wavelength Laser Aiming System: Allows for successful t
The shortening of the	wavelength led Townes and his colleagues to focus on mi
nd therefore have energies above 100 keV and	wavelength less than 10 picometers, less than the diame
The tunable laser provides a narrow, tunable	wavelength light source that can be used to analyze the
at room light does not contain the UV (short	wavelength light) found in sunlight.
When excited with 488 nm	wavelength light, it fluoresces red.
ng background geometry, the low energy large	wavelength limit of the theory has to decouple from the
The short	wavelength limit of QCLs is determined by the depth of
etimes taken is to only consider the largest	wavelength modes of the order of the size of the univer
Parabolas only focus waves with a	wavelength much smaller than the diameter of the parabo
method of stereoscopic projection is called	wavelength multiplex visualization.
	Wavelength multiplexing techniques.
reads or counts only the x-rays of a single	wavelength, not producing a broad spectrum of wavelengt
anged as an interferometer for submillimeter	wavelength observations.
A reference	wavelength of 589.3 nm (the sodium D line) is most ofte
The physical	wavelength of a perturbation mode (dashed line) is also
lectromagnetic irradiation (usually a single	wavelength of visible or UV light).
Pure GaP LEDs emit green light at a	wavelength of 555 nm.
When excited by a specific	wavelength of light, the protein will fluoresce.
where λ is the	wavelength of the spectral peak of interest and
y the result of color filters that alter the	wavelength of the light prior to exiting the endoderm,
0 the refractive index of the solvent, λ the	wavelength of the light source, dn/dc the refactive ind
tandard colourimeters cannot operate below a	wavelength of 400 nanometers.
absorption spectroscopy, corresponding to a	wavelength of maximum absorption.
ially broadcast on 104.3 MHz and 1170 kHz (a	wavelength of 257 metres, with the phrase "2 5 7" becom
DNA absorbs UV light with a	wavelength of maximal absorbance near 260 nm.
stronomy), due to atomic oxygen, occurs at a	wavelength of 5577 angstroms (557.7 nanometers).
The maximum efficacy is 683 lm/W at a	wavelength of 555 nm (green).
should be at least ten times longer than the	wavelength of interesting features.
However, the	wavelength of visible light (about 4000 to 7000 angstro
ttering reduces the energy (or increases the	wavelength) of the outgoing beam.
mitting an excess of infrared radiation at a	wavelength of 70 μm.
The	wavelength of the impinging x-ray and the crystal's lat
ency conversion involves the shifting of the	wavelength of a monochromatic source of light, usually
s strongly influenced by temperature and the	wavelength of light used to measure it, therefore, care
planes of spheres is approximately half the	wavelength of a component of visible light, the light o
applications for selection of the excitation	wavelength of light from a light source.
ange can be read on a spectrophotometer at a	wavelength of 370 or 655 nm.
neutron and X-ray optics to select a defined	wavelength of the radiation for further purpose on a de
Because the	wavelength of light selected by the filter varies with
in both continuous and pulsed mode, and the	wavelength of the laser beam is 10.6 μm.
ree path of an atom is much smaller than the	wavelength of the radiative transition, the atom change
this will produce an echo with a maximum	wavelength of that order, which corresponds to a freque
ing the red-shift of galaxies - the shift in	wavelength of light to longer wavelengths due to a spee
ermolysis (SPTL), the matching of a specific	wavelength of light and pulse duration to obtain optima
Because the	wavelength of light determines its color, the variation
fringes with a spacing of , with λ being the	wavelength of the beam, n being the refractive index an
ation about layers that are thinner than the	wavelength of the probing light itself, even down to a
e lowest possible BPP, λ / π, where λ is the	wavelength of the light.
At a	wavelength of 260 nm, the average extinction coefficien
ough at least one filter above and below the	wavelength of the redshifted Lyman break.
e d is the resolvable feature size, λ is the	wavelength of light, n is the index of refraction of th
1 at 300 K. Its refractive index is 3.3 at a	wavelength of 2 µm, and its dielectric constant is 10.9
ydrogen, the deuterium fluoride lases at the	wavelength of about 3.8 µm.
s on the scatterer or medium relative to the	wavelength of the scattered particles.
icles in question are similar in size to the	wavelength of the laser.
h about 0.25 ns) at its fundamental emission	wavelength of 1.315 micrometers.
4 eV at 300 K, which corresponds to infrared	wavelength of about 860 nm) out to wavelengths greater
ing in sharp resonances in the intensity and	wavelength of the photoluminescence.
e de Broglie relation, a beam of 54 eV had a	wavelength of 0.165 nm.
source brightness, and the short De Broglie	wavelength of the helium ions, which is inversely propo
he optical density of a sample measured at a	wavelength of 600 nm.
ated with an infrared laser operating at the	wavelength of 16 µm.
h of about 1 ns) at its fundamental emission	wavelength of 1.315 micrometers, though it is also capa
tails often contain additives that shift the	wavelength of the emitted light to make it more easily
The exact	wavelength of this threshold is redshifted and can be u
on), the eye is most sensitive to light at a	wavelength of 555 nm.
ground state by emission of a photon at the	wavelength of 600 nm.
d to as L37 or L39 filters, depending on the	wavelength of light that they filter out; an L37 filter
g by particles similar to or larger than the	wavelength of light is typically treated by the Mie the
Under laser irradiation at a	wavelength of less than 520 nm, it decomposes to pluton
objective, and inversely proportional to the	wavelength of the light being observed.
er signal, as a function of the frequency or	wavelength of the signal.
n the far infrared region (about 30 - 150 µm	wavelength) of the electromagnetic spectrum.
rotation of a substance with a change in the	wavelength of light.
with a laser, and subsequently analyzing the	wavelength of emitted light.
Diffraction occurs because the	wavelength of electrons accelerated by a potential of a
by measuring the absorbance of a particular	wavelength of light by the sample and how it changes ov
e star is 8th magnitude at the near infrared	wavelength of 2 micrometers, it is calculated to be abo
oscillation", with an accretion and breakup	wavelength of ~500 million years, stretching all the wa
site using four filters: Blue (with a center	wavelength of 435 nm), Visual (555 nm), Infrared (814 n
s invisible to the human eye by changing the	wavelength of reflected light.
is image is inaccurate because the different	wavelength of different colors of light cause them to r
etermined by the prisms' wedge angle and the	wavelength of the light.
lly at a frequency of 2.45 gigahertz (GHz)-a	wavelength of 122 millimetres (4.80 in)-through the foo
to scatter electromagnetic radiation if the	wavelength of the light is similar to the size of the d
e of the density fluctuations approaches the	wavelength of light, the light is scattered and causes
riod of the diffraction grating and λ is the	wavelength of the light incident on the grating.
nuously with output power of over 100 mW and	wavelength of 9.5 µm.

1 2 次へ＞

共起表現

「Wavelength」の共起表現(1語右で並び替え) - Weblio英語共起表現検索

「Wavelength」の共起表現一覧(1語右で並び替え)