「Wavelength」の共起表現一覧(2語左で並び替え)
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A reference | wavelength of 589.3 nm (the sodium D line) is most ofte |
lectromagnetic irradiation (usually a single | wavelength of visible or UV light). |
When excited by a specific | wavelength of light, the protein will fluoresce. |
wo laser sources that operate at a different | wavelength. |
exit slits, each of which allows a different | wavelength to pass through it. |
In 1962, a longer | wavelength radar, 10-cm, was constructed and designated |
ossible lattice vibration has a well-defined | wavelength and frequency. |
t landslide-triggered tsunamis have a larger | wavelength than earthquake-generated tsunamis, which su |
imen is illuminated with light of a specific | wavelength (or wavelengths) which is absorbed by the fl |
orbance of the sample solution at a specific | wavelength to a series of standard solutions at differi |
ill produce when illuminated by a particular | wavelength. |
reads or counts only the x-rays of a single | wavelength, not producing a broad spectrum of wavelengt |
efers to absorptance measured at a specified | wavelength. |
he fraction of radiation absorbed at a given | wavelength. |
neutron and X-ray optics to select a defined | wavelength of the radiation for further purpose on a de |
this will produce an echo with a maximum | wavelength of that order, which corresponds to a freque |
Communications were via a decimeter | wavelength radio transmitter mounted in the orbital mod |
ermolysis (SPTL), the matching of a specific | wavelength of light and pulse duration to obtain optima |
from Oliphant, who wanted to develop a small | wavelength radiation generator, Titterton worked as a r |
There is a musical | wavelength to what he does," said Corea to The San Dieg |
aterials, M(λ) approaches zero at a specific | wavelength λ0 between 1.3 and 1.5 μm. |
At wavelengths as short as 157 nm, a common | wavelength used for semiconductor stepper manufacture f |
intensity falls off sharply above a specific | wavelength. |
adiation emitted by X-ray tubes had a longer | wavelength than the radiation emitted by radioactive nu |
nfrared detectors, each sensing a particular | wavelength, a temperature profile, or sounding of the a |
adiations, in which a photon of a particular | wavelength is absorbed and an equivalent photon is imme |
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 |
or holes) generated for a photon of a given | wavelength, QE. |
by measuring the absorbance of a particular | wavelength of light by the sample and how it changes ov |
site using four filters: Blue (with a center | wavelength of 435 nm), Visual (555 nm), Infrared (814 n |
emission spectrum of a molecule to a longer | wavelength (lower frequency).. |
Submillimeter Telescope, is a submillimeter | wavelength radio telescope located on Mount Graham, Ari |
color is a color that is evoked by a single | wavelength of light in the visible spectrum, or by a re |
Unlike an x-ray photon with a similar | wavelength, which interacts with the electron cloud sur |
a chemical species absorbs light at a given | wavelength. |
e photophore is believed to be of a specific | wavelength, possibly both preventing miscommunication a |
frequency of a standing wave where a quarter | wavelength is the distance between the base of the mug |
, and moderately low dispersion over a wider | wavelength range than a singly clad fiber or a doubly c |
But when activated by light of a certain | wavelength, it has a major impact on the cornea," NBC's |
So it is a half | wavelength out of phase with the first wave when they c |
d color in the visible spectrum has a higher | wavelength than most other colors, this effect is also |
ntangled photons to function as if a shorter | wavelength was used to allow detection of small details |
hould not only absorb laser light of a given | wavelength, but they should also be able to withstand a |
This was supplemented by a meter | wavelength range transmitter through the omnidirectiona |
This luciferase reaction has a peak | wavelength of about 490 nm. |
gram) around any point O on the face AB, the | wavelength which is deviated by 60° can be selected. |
this general shape are absorption features ( | wavelength bands where the intensity is lowered) that h |
So it is actually the | wavelength which is affected; as a consequence, the rec |
All other | wavelength ranges of the spectrum are reflected, scatte |
The TAMU-1 was updated in 1966 to allow dual | wavelength operations. |
ptical telecommunications, allowing all-band | wavelength coverage and in-line distributed signal ampl |
y the result of color filters that alter the | wavelength of the light prior to exiting the endoderm, |
e telemetric data at the 70 cm amateur radio | wavelength (437.345 |
with a laser, and subsequently analyzing the | wavelength of emitted light. |
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. |
s strongly influenced by temperature and the | wavelength of light used to measure it, therefore, care |
in both continuous and pulsed mode, and the | wavelength of the laser beam is 10.6 μm. |
otoluminescence at room temperature, and its | wavelength and lifetime can be tuned by substitution of |
oscillation", with an accretion and breakup | wavelength of ~500 million years, stretching all the wa |
etermined by the prisms' wedge angle and the | wavelength of the light. |
probing beam has ~500-fs duration, and ~1-μm | wavelength. |
cribes an approach, rather than any specific | wavelength range, multivariate optical computers may be |
e of the density fluctuations approaches the | wavelength of light, the light is scattered and causes |
n be transferred by an optical fiber, as its | wavelength is not absorbed much by fused silica but is |
the optical rotation first increases as the | wavelength decreases (as first observed by Cotton), and |
However, as shorter | wavelength continuous spectrum "X-ray" sources such as |
It is used as a | wavelength shifter (also called a "secondary scintillat |
Pure GaP LEDs emit green light at a | wavelength of 555 nm. |
antennas simultaneously observing at 10.7-cm | wavelength. |
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). |
mitting an excess of infrared radiation at a | wavelength of 70 μm. |
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. |
o that the dispersion curves coincide at one | wavelength. |
At a | wavelength of 260 nm, the average extinction coefficien |
ed after each slit so that the light at each | wavelength is measured by a different detector. |
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. |
more luminous than our local star at visible | wavelength. |
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. |
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. |
Under laser irradiation at a | wavelength of less than 520 nm, it decomposes to pluton |
how a drop in the continuum radiation at the | wavelength associated with the absorbed photons. |
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 |
Regular KDP has absorbances at this | wavelength of around 4.7-6.3%/cm of thickness while hig |
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. |
Hydrogen fluoride lasers operate at the | wavelength of 2.7-2.9 µm. |
The horizontal axis is | wavelength in nm. |
erman countermeasure to SHF band centimetric | wavelength radar produced by a cavity magnetron. |
romator before reading it in narrow bands of | wavelength. |
uced from the short-pulse beam's fundamental | wavelength (1053 nm) at the target/plasma/laser interfa |
Because the | wavelength of light selected by the filter varies with |
Because the | wavelength of light determines its color, the variation |
Diffraction occurs because the | wavelength of electrons accelerated by a potential of a |
produce a diffraction pattern because their | wavelength is typically the same order of magnitude (0. |
fringes with a spacing of , with λ being the | wavelength of the beam, n being the refractive index an |
tandard colourimeters cannot operate below a | wavelength of 400 nanometers. |
ough at least one filter above and below the | wavelength of the redshifted Lyman break. |
optic cable absorbs and is destroyed by this | wavelength, so a rigid lens and mirror delivery system |
r systems are differentiated not only by the | wavelength, but also by the light delivery system: flex |
This causes the | wavelength λ to decrease, which means that the signal t |
monochromatic light could also change their | wavelength (the Cabannes-Daure effect). |
s invisible to the human eye by changing the | wavelength of reflected light. |
of radiation, a monochromator to choose the | wavelength, slits to adjust the shape of the beam, a sa |
45, 14.9 and 32.5 GHz (i.e. 3, 2 and 1 cm in | wavelength) at the Teide Observatory, Tenerife. |
elocity of the wave remains constant whereas | wavelength changes; hence frequency also changes. |
nterferometers due to their short de Broglie | wavelength. |
source brightness, and the short De Broglie | wavelength of the helium ions, which is inversely propo |
esents refractive index, the "D" denotes the | wavelength, and the 20 denotes the reference temperatur |
a, the index of refraction is dependent upon | wavelength. |
This absorption depends on | wavelength. |
-rich areas of the sky in terms of depth and | wavelength coverage. |
may be needed to select the desired neutron | wavelength. |
W0 is defined as the difference in | wavelength between the points on either side of the emi |
be recorded sequentially at different narrow | wavelength bands. |
or one instrument both energy dispersive and | wavelength dispersive instrumentation is available prov |
Each infrared | wavelength is sensitive to temperature and water vapor |
ptical switching, electro-optical switching, | wavelength conversion, reconfigurable optical delay lin |
ng background geometry, the low energy large | wavelength limit of the theory has to decouple from the |
rectangular waveguide with equivalent guided | wavelength. |
ily cascaded, thus accessing essentially any | wavelength in the fiber low-loss guiding windows (both |
53 cm (553 to 566 MHz) - an extremely short | wavelength for the time - with a pulse length of 2 micr |
hrop Grumman's LLDR, using an eye-safe laser | wavelength, recognizes targets, finds the range to a ta |
roject which demonstrated the feasibility of | wavelength routed optical networks that are now being i |
id-state Er:YAG lasers, which also feature a | wavelength that is highly absorbed by water. |
D for direct imaging and a fiber-fed visible | wavelength spectrograph, FOBOS, for general spectroscop |
ter Imager observes the sun in five distinct | wavelength, 220, 279.2, 300, 323 and 388 nm, on a 2048 |
The laser radiation can be fixed in | wavelength such as that of an argon ion laser or that o |
For this | wavelength the filled optical cell behaves like a plane |
anged as an interferometer for submillimeter | wavelength observations. |
(FSR) is the spacing in optical frequency or | wavelength between two successive reflected or transmit |
er signal, as a function of the frequency or | wavelength of the signal. |
nox radiator is related to the frequency (or | wavelength) of the service transmitted, and for maximum |
aphs, which measure photons as a function of | wavelength or frequency, with typical resolution on the |
on properties of a material as a function of | wavelength. |
e transmission of an etalon as a function of | wavelength. |
ron, to a quantum of light, as a function of | wavelength. |
th harmonics of the Nd:YAG fundamental laser | wavelength (1064 nm). |
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 |
lly at a frequency of 2.45 gigahertz (GHz)-a | wavelength of 122 millimetres (4.80 in)-through the foo |
e de Broglie relation, a beam of 54 eV had a | wavelength of 0.165 nm. |
esults, the antennas should be spaced half a | wavelength apart, or less. |
planes of spheres is approximately half the | wavelength of a component of visible light, the light o |
th a height corresponding to a half radiated | wavelength was Warsaw Radio Mast. |
ing at 344 m/s and the corrugated iron has a | wavelength (pitch) of 3” or .0762m |
However, the | wavelength of visible light (about 4000 to 7000 angstro |
to scatter electromagnetic radiation if the | wavelength of the light is similar to the size of the d |
te glass retains useful transmission in this | wavelength region, allowing large aperture optics to be |
ess at the biosensor tip, which results in a | wavelength shift, Δλ (Figure 3), which is a direct meas |
e telescope is intended to observe in longer | wavelength infrared than the James Webb Space Telescope |
rotation of a substance with a change in the | wavelength of light. |
urance method, to verify the accuracy in the | wavelength of a spectrophotometer. |
In a | wavelength region where the light is absorbed, the abso |
factured to operate most efficiently in that | wavelength range. |
aphy to monitor small deformations in single | wavelength implementations as well as dimensional metro |
em of the chromophore, they may increase the | wavelength at which the light is absorbed and as a resu |
s is achieved by using the increased Compton | wavelength, which is just the Compton wavelengths of th |
ttering reduces the energy (or increases the | wavelength) of the outgoing beam. |
than λ0, M(λ) is negative and increases with | wavelength; at wavelengths longer than λ0, M(λ) is posi |
ich the computational cost is independent of | wavelength. |
ing in sharp resonances in the intensity and | wavelength of the photoluminescence. |
ea of the line on a plot of intensity versus | wavelength. |
arameters of fluorescence: its intensity and | wavelength distribution of emission spectrum after exci |
rometers and a few millimeters, which is the | wavelength range in which the SMA can observe. |
where λ is the | wavelength of the spectral peak of interest and |
where λ is the | wavelength, f is the frequency, and c is the speed of p |
The end result is the | wavelength spectrum in the vertical direction for each |
e lowest possible BPP, λ / π, where λ is the | wavelength of the light. |
e d is the resolvable feature size, λ is the | wavelength of light, n is the index of refraction of th |
riod of the diffraction grating and λ is the | wavelength of the light incident on the grating. |
Where λg is the | wavelength corresponding to the central rejection frequ |
is the | wavelength of the wave. |
ce from pinhole to image plane) and λ is the | wavelength of light. |
method of stereoscopic projection is called | wavelength multiplex visualization. |
or the diametre of the antenna) and λ is the | wavelength of the radio wave. |
ere D00 is the beam waist size, and λ is the | wavelength. |
also absorbs some of the light at its lasing | wavelength. |
s depends on the instrument and its spectral | wavelength, the measuring or scanning method, the time |
the team that investigated Jupiter's visible | wavelength response to the impact of comet Shoemaker-Le |
nd therefore have energies above 100 keV and | wavelength less than 10 picometers, less than the diame |
ially broadcast on 104.3 MHz and 1170 kHz (a | wavelength of 257 metres, with the phrase "2 5 7" becom |
eter mediumwave band (1500 kHz)-the shortest | wavelength then available to amateurs. |
parameters (dose, type of laser, materials, | wavelength, etc.) have not been identified. |
ch is reflected from a surface) for light of | wavelength 540 nm varies between 29.6 and 30.2, and is |
of photosynthesis after exposure to light of | wavelength 670 nm and 700 nm, respectively. |
Ernst Abbe found in 1873 that light with | wavelength λ,travelling in a medium with refractive ind |
ted with respect to the spectral line's rest | wavelength. |
Also, the applied field is longer in | wavelength than the lattice spacing. |
tion) the remaining power at longer infrared | wavelength contained basically two components: the CIB |
he serial that ran on Radio Luxembourg's 208 | wavelength. |
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