「Wavelength」の共起表現一覧(1語左で並び替え)
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ws to use an intense beam of neutrons with a | wavelength distribution of 10% or more and at the same |
Pure GaP LEDs emit green light at a | wavelength of 555 nm. |
tandard colourimeters cannot operate below a | wavelength of 400 nanometers. |
absorption spectroscopy, corresponding to a | wavelength of maximum absorption. |
DNA absorbs UV light with a | wavelength of maximal absorbance near 260 nm. |
eed, oxygen gas absorbs the radiation with a | wavelength below 195 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). |
Glass, with a | wavelength from 380 to 780 nm (visible spectrum) |
Plastic, with a | wavelength from 380 to 780 nm (visible spectrum) |
Parabolas only focus waves with a | wavelength much smaller than the diameter of the parabo |
ncy downshift of ~11 THz (corresponding to a | wavelength shift at ~1550 nm of ~90 nm). |
mitting an excess of infrared radiation at a | wavelength of 70 μm. |
esults, the antennas should be spaced half a | wavelength apart, or less. |
xt is 120° (2π/3 radians), or one third of a | wavelength λ/3. |
microseconds, de-excite and emit light at a | wavelength larger than the excitation wavelength. |
ange can be read on a spectrophotometer at a | wavelength of 370 or 655 nm. |
lescopes to be positioned to a fraction of a | wavelength). |
At a | wavelength of 260 nm, the average extinction coefficien |
1 at 300 K. Its refractive index is 3.3 at a | wavelength of 2 µm, and its dielectric constant is 10.9 |
ess at the biosensor tip, which results in a | wavelength shift, Δλ (Figure 3), which is a direct meas |
the anomalous dispersion that occurs when a | wavelength is selected that is in the vicinity of an ab |
e de Broglie relation, a beam of 54 eV had a | wavelength of 0.165 nm. |
he optical density of a sample measured at a | wavelength of 600 nm. |
This laser beam is tuned to a | wavelength that causes the hydroxyl molecules to fluore |
on), the eye is most sensitive to light at a | wavelength of 555 nm. |
ing at 344 m/s and the corrugated iron has a | wavelength (pitch) of 3” or .0762m |
Under laser irradiation at a | wavelength of less than 520 nm, it decomposes to pluton |
id-state Er:YAG lasers, which also feature a | wavelength that is highly absorbed by water. |
nsitions upon the absorption of light with a | wavelength of 314.5 nm. |
icient of approximately 13.2 X 10−6 m−1 at a | wavelength of 520 nm. |
Chlorophyll a absorbs well at a | wavelength of about 400-450 nm and at 650-700 nm; chlor |
It is used as a | wavelength shifter (also called a "secondary scintillat |
At a | wavelength of 5 μm, it was found to have the highest fl |
evealed an excess of infrared radiation at a | wavelength of 160 μm. |
surrounds the galaxies absorbs light with a | wavelength around 100 nanometers, the galaxies have a n |
Fused quartz, with a | wavelength below 380 nm (ultraviolet spectrum) |
It absorbs light with a | wavelength of 320 nm and emits light with a wavelength |
In a | wavelength region where the light is absorbed, the abso |
phase and amplitude elements smaller than a | wavelength of light. |
Er:YAG lasers typically emit light with a | wavelength of 2940 nm, which is infrared light. |
of a physiological activity plotted against | wavelength of light. |
ptical telecommunications, allowing all-band | wavelength coverage and in-line distributed signal ampl |
photons have the same energy (frequency) and | wavelength as the incident photons. |
-rich areas of the sky in terms of depth and | wavelength coverage. |
ing in sharp resonances in the intensity and | wavelength of the photoluminescence. |
or one instrument both energy dispersive and | wavelength dispersive instrumentation is available prov |
nuously with output power of over 100 mW and | wavelength of 9.5 µm. |
nd therefore have energies above 100 keV and | wavelength less than 10 picometers, less than the diame |
arameters of fluorescence: its intensity and | wavelength distribution of emission spectrum after exci |
its active phased array X-band SAR antenna ( | wavelength 31 mm, frequency 9.6 GHz), TerraSAR-X acquir |
ily cascaded, thus accessing essentially any | wavelength in the fiber low-loss guiding windows (both |
en the same number of photons of appropriate | wavelength. |
When light of the appropriate | wavelength is coupled to the loop by the input waveguid |
ty of tunable laser light at the appropriate | wavelength and also the availability of high reflectanc |
Frog Eyes performed at | Wavelength #177 in August 2003 (Wavelength Music Arts P |
omagnetic energy being received on the BBC's | wavelength when the plane flew overhead, and thus radio |
or Soret Band is an intense peak in the blue | wavelength region of the visible spectrum. |
oscillation", with an accretion and breakup | wavelength of ~500 million years, stretching all the wa |
l, Plymouth Evening Herald, The West Briton, | Wavelength, Cornwall Today magazine, Brides in Cornwall |
nterferometers due to their short de Broglie | wavelength. |
source brightness, and the short De Broglie | wavelength of the helium ions, which is inversely propo |
Both series' were produced by | Wavelength Films for ITV London, and series one was als |
method of stereoscopic projection is called | wavelength multiplex visualization. |
site using four filters: Blue (with a center | wavelength of 435 nm), Visual (555 nm), Infrared (814 n |
An 8 centimeter | wavelength transmitter mounted in the experiment module |
evelop a radar system with a 1.25 centimeter | wavelength. |
erman countermeasure to SHF band centimetric | wavelength radar produced by a cavity magnetron. |
ission from a blackbody that is in a certain | wavelength interval or band. |
can be quantified by measuring at a certain | wavelength (usually between 500 and 600 nm) by a spectr |
But when activated by light of a certain | wavelength, it has a major impact on the cornea," NBC's |
de more effective by including Grom-2 (10 cm | wavelength) radars to the AA-batteries. |
es the frequency between 5600-5650 MHz (5 cm | wavelength) carrier wave, with an angular resolution be |
version, the S-band (2500-3700 MHz, 12-9 cm | wavelength) FuMB7 Naxos U, was provided to U-boats to a |
.8 m solar flux monitor observing at 10.7 cm | wavelength. |
At wavelengths as short as 157 nm, a common | wavelength used for semiconductor stepper manufacture f |
a black hole is roughly equal to the Compton | wavelength at the Planck scale, a photon with sufficien |
is the Compton | wavelength of the proton. |
s is achieved by using the increased Compton | wavelength, which is just the Compton wavelengths of th |
d to Ga it is possible to extend the cut-off | wavelength up to about 2.6 µm. |
Communications were via a decimeter | wavelength radio transmitter mounted in the orbital mod |
he first Russian radar to use the decimetric | wavelength, the first prototype being created in 1947, |
neutron and X-ray optics to select a defined | wavelength of the radiation for further purpose on a de |
ed to filter neutron pulses with the desired | wavelength. |
nk that the chirp starts outside the desired | wavelength range, and any wavelength within the range e |
web camera can be used for video detection ( | wavelength between 0.4 and 0.7 µm). |
wo laser sources that operate at a different | wavelength. |
exit slits, each of which allows a different | wavelength to pass through it. |
pt that it applies to functions of different | wavelength. |
is image is inaccurate because the different | wavelength of different colors of light cause them to r |
t such depths, sunlight has a very different | wavelength profile than at the surface, so isorenierate |
al version operating on a slightly different | wavelength was also developed as Seetakt. |
ter Imager observes the sun in five distinct | wavelength, 220, 279.2, 300, 323 and 388 nm, on a 2048 |
The TAMU-1 was updated in 1966 to allow dual | wavelength operations. |
TD 110 Dual | wavelength Laser Aiming System: Allows for successful t |
ed after each slit so that the light at each | wavelength is measured by a different detector. |
Each | wavelength of light has its own 'event horizon', inside |
'capacity hat', which extends the electrical | wavelength, at the top. |
h about 0.25 ns) at its fundamental emission | wavelength of 1.315 micrometers. |
h of about 1 ns) at its fundamental emission | wavelength of 1.315 micrometers, though it is also capa |
Additionally, the peak emission | wavelength is about 480 nm. |
The emission | wavelength can be lowered by substituting the anthracen |
λ represents the intensity across the entire | wavelength range of interest. |
gth among the rays diffracted, even of equal | wavelength. |
Every | wavelength of light is perceived as a spectral color, i |
The exact | wavelength of this threshold is redshifted and can be u |
tage of fluorospheres is that the excitation | wavelength and the emission wavelength are not the same |
applications for selection of the excitation | wavelength of light from a light source. |
ite laser light into the required excitation | wavelength (selected for by a narrow slit)]. |
orescence microscopy in which the excitation | wavelength is shorter than the emission wavelength, as |
1,5-IAEDANS has a peak excitation | wavelength of 336 nm and a peak emission wavelength of |
xpressed in wavenumber, λ0 is the excitation | wavelength, and λ1 is the Raman spectrum wavelength. |
this general shape are absorption features ( | wavelength bands where the intensity is lowered) that h |
To get a single and fixed | wavelength at the end station, a monochromator is used. |
half-wavelength past the load; this flexural | wavelength is determined in large part by the elastic t |
e, Part One" were used in the soundtrack for | Wavelength. |
uced from the short-pulse beam's fundamental | wavelength (1053 nm) at the target/plasma/laser interfa |
he fraction of radiation absorbed at a given | wavelength. |
or holes) generated for a photon of a given | wavelength, QE. |
a chemical species absorbs light at a given | wavelength. |
hould not only absorb laser light of a given | wavelength, but they should also be able to withstand a |
rectangular waveguide with equivalent guided | wavelength. |
So it is a half | wavelength out of phase with the first wave when they c |
yellow light from a sodium source, that has | wavelength 589.3 nanometres. |
d color in the visible spectrum has a higher | wavelength than most other colors, this effect is also |
Also, the applied field is longer in | wavelength than the lattice spacing. |
capture data in 36 spectral bands ranging in | wavelength from 0.4 µm to 14.4 µm and at varying spatia |
very organism's bioluminescence is unique in | wavelength, duration, timing and regularity of flashes. |
W0 is defined as the difference in | wavelength between the points on either side of the emi |
ing the red-shift of galaxies - the shift in | wavelength of light to longer wavelengths due to a spee |
However, when used in | wavelength division multiplexing systems, dispersion-sh |
45, 14.9 and 32.5 GHz (i.e. 3, 2 and 1 cm in | wavelength) at the Teide Observatory, Tenerife. |
The laser radiation can be fixed in | wavelength such as that of an argon ion laser or that o |
Small changes of the incident | wavelength generated by an acousto-optic modulator or i |
is the incident | wavelength. |
e refractive index decreases with increasing | wavelength. |
tion) the remaining power at longer infrared | wavelength contained basically two components: the CIB |
iode lasers in the visible and near infrared | wavelength range (600-2,000 nm), the Carbon dioxide or |
n the ultraviolet, visible and near infrared | wavelength region (240 nm - 2380 nm) at moderate spectr |
4 eV at 300 K, which corresponds to infrared | wavelength of about 860 nm) out to wavelengths greater |
Each infrared | wavelength is sensitive to temperature and water vapor |
e star is 8th magnitude at the near infrared | wavelength of 2 micrometers, it is calculated to be abo |
r is identical, or is one (or other integer) | wavelength apart. |
This condition is met in the IR-visible | wavelength region for air/metal and water/metal interfa |
se to familiar absorption of light, which is | wavelength dependent and gives rise to colours. |
The horizontal axis is | wavelength in nm. |
e extent of rotation of light depends on its | wavelength. |
n be transferred by an optical fiber, as its | wavelength is not absorbed much by fused silica but is |
otoluminescence at room temperature, and its | wavelength and lifetime can be tuned by substitution of |
for the discrimination of light based on its | wavelength components. |
omentum of the particle p was related to its | wavelength λ by what is now known as the de Broglie rel |
e strongly confined) than about one-half its | wavelength, λ. |
d through a filter creating a light of known | wavelength which is then passed through a cuvette conta |
ng background geometry, the low energy large | wavelength limit of the theory has to decouple from the |
t landslide-triggered tsunamis have a larger | wavelength than earthquake-generated tsunamis, which su |
ange of a diffraction grating is the largest | wavelength range for a given order that does not overla |
etimes taken is to only consider the largest | wavelength modes of the order of the size of the univer |
hrop Grumman's LLDR, using an eye-safe laser | wavelength, recognizes targets, finds the range to a ta |
th harmonics of the Nd:YAG fundamental laser | wavelength (1064 nm). |
delay time of the acceleration power, laser | wavelength, energy density of the laser and the impact |
lasing mode confined to 1/100th of the laser | wavelength. |
f energy absorbed is a function of the laser | wavelength. |
pulsed lasers, time domain optimized lasers, | wavelength adapted lasers, and ultra compact modular la |
also absorbs some of the light at its lasing | wavelength. |
Enabled Radar - TRACER is a mid-range, long | wavelength synthetic aperture radar (SAR) system that p |
These arrays are simple long | wavelength telescopes that hope to detect the redshifte |
They are focused largely on long | wavelength protease assays. |
The Long | Wavelength Array (LWA) is a radio telescope under const |
orhodopsin, is actually opaque to the longer | wavelength ultraviolet (its red color). |
In 1962, a longer | wavelength radar, 10-cm, was constructed and designated |
e telescope is intended to observe in longer | wavelength infrared than the James Webb Space Telescope |
adiation emitted by X-ray tubes had a longer | wavelength than the radiation emitted by radioactive nu |
emission spectrum of a molecule to a longer | wavelength (lower frequency).. |
es fluorescence is the re-emission of longer | wavelength photons (lower frequency or energy) by a mol |
offset by the extra distance that the longer | wavelength components have to travel through the second |
It operates at 81.5 MHz (3.7 m | wavelength), and is made up of 4096 dipoles in a phased |
parameters (dose, type of laser, materials, | wavelength, etc.) have not been identified. |
this will produce an echo with a maximum | wavelength of that order, which corresponds to a freque |
The detectors were designed to measure | wavelength and flux shifts of solar radiation during pe |
The SCR-68 operated at 750 kHz (400 meter | wavelength), using a long wire antenna reeled out behin |
This was supplemented by a meter | wavelength range transmitter through the omnidirectiona |
at the fundamental line of 1.315 micrometres | wavelength with a total energy of about 1 kilojoule (or |
it emits radiation from 4 to 15 micrometres | wavelength. |
continuously measured at single or multiple | wavelength. |
There is a musical | wavelength to what he does," said Corea to The San Dieg |
n of dibromodifluoromethane at 248 nanometer | wavelength. |
For ozone, a 254 nanometer | wavelength of light created by a mercury lamp is shined |
be recorded sequentially at different narrow | wavelength bands. |
egral) and to the third power of the neutron | wavelength. |
may be needed to select the desired neutron | wavelength. |
It absorbs far-red light, at 710 nm | wavelength, just outside the optical range. |
When excited with 488 nm | wavelength light, it fluoresces red. |
tion of a red colouration (peaking at 580 nm | wavelength) when chromotropic acid in 75% sulfuric acid |
ors detect light intensity with little or no | wavelength specificity, and therefore cannot separate c |
GHz radiometer according to their observing | wavelength to obtain the same response on sky: three fi |
ich the computational cost is independent of | wavelength. |
roject which demonstrated the feasibility of | wavelength routed optical networks that are now being i |
fields within astronomy, using wide range of | wavelength in observation. |
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