「wavelengths」の共起表現一覧(1語右で並び替え)
該当件数 : 205件
Since holograms reflect light at certain | wavelengths a change in their composition can generate |
pool cause refracted light to lose certain | wavelengths, a distinct yellow-green hue is noticeable. |
g device, usually a CCD camera sensitive to | wavelengths above the normal "visible" (0.4 to 0.7 micr |
r - measures tropospheric ozone in infrared | wavelengths, also carbon monoxide, methane and nitrogen |
rometric astronomical measurements at radio | wavelengths, although it is claimed that Joseph Pawsey |
r, the normal modes do possess well-defined | wavelengths and frequencies. |
or reflectivity at the shortest ultraviolet | wavelengths, and two mirror segments are coated with li |
ultiwavelength pyrometers use three or more | wavelengths and mathematical manipulation of the result |
By employing several | wavelengths and time resolved (frequency or time domain |
ed by the size of the synthetic aperture in | wavelengths, and cannot be finer than the system's reso |
molecules to obtain even shorter de Broglie | wavelengths and to search for the limits of quantum mec |
mes more sensitive than IRAS at the shorter | wavelengths, and also had an extended mission into 2011 |
eptional stability and efficiency for short | wavelengths, and it almost immediately appeared in high |
Other | wavelengths are deflected at angles dependent about the |
of refraction, layer thicknesses and light | wavelengths, are assumed constant with some uncertainty |
spectrum; the colors of sufficiently close | wavelengths are indistinguishable. |
ral gabrielite is not pleochroic (different | wavelengths are absorbed in different directions, the c |
Short | wavelengths are rotated more than longer wavelengths. |
Thus, if the source | wavelengths are λ1 and λ2, the resulting wavelength is |
filter allows transmission of both deep-red | wavelengths around 690 nanometres and yellow-green wave |
w amino acids and absorb light at different | wavelengths as retinal-bound pigments. |
ells 2.1 eV deep and electroluminescence at | wavelengths as short as 2.5 μm has been observed. |
s and release the energy at longer infrared | wavelengths as photographed by the Spitzer Space Telesc |
At | wavelengths as short as 157 nm, a common wavelength use |
are more specific in terms of the range of | wavelengths at which quantum yields have been determine |
n exposed the plants to both short and long | wavelengths at the same time, causing the efficiency to |
lable in the later reprints), and tables of | wavelengths at which various materials absorbed IR ligh |
ding approximately 50 of its 544 measurable | wavelengths at a resolution of 100 to 200 meters per pi |
s coefficient is unity for a narrow band of | wavelengths at 555 nanometres. |
nisms require that light of the appropriate | wavelengths be absorbed within the active area of chlor |
possible deviation of the prism, all other | wavelengths being deviated by greater angles. |
a UVB absorber, meaning that it can absorb | wavelengths between 290-320 nm. |
rence makes chlorophyll b absorb light with | wavelengths between 400 and 500 nm more efficiently. |
ximum baseline of 32 meters and operated in | wavelengths between 450 and 800 nm. |
It is highly transparent for | wavelengths between 350-2700 nm with a reduced transmis |
s between 210 and 880 GHz, corresponding to | wavelengths between 0.35 and 1.4mm, for observations of |
pically emit the bulk of their radiation at | wavelengths between a few hundred micrometers and a few |
e for research in astronomy and aeronomy at | wavelengths between 0.2 and 2 mm. |
on the fact that bilirubin absorbs light of | wavelengths between 450-460 nm. |
It emits | wavelengths between 382-622 nm, though the primary emis |
e designed to block or reflect mid-infrared | wavelengths but pass visible light. |
lse amplifiers are often converted to other | wavelengths by means of various nonlinear optics proces |
curing material was first measured at radio | wavelengths by the VLBA and VLA. |
r light source that emits light of variable | wavelengths by an optical parametric amplification proc |
rts of it are obscured from view in visible | wavelengths by regions of cosmic dust. |
It was first detected at radio | wavelengths by radiation from the 21 cm emission line o |
e burst's afterglow was detected in optical | wavelengths by the Mercator Telescope, radio wavelength |
Image formation, normally done at optical | wavelengths by lenses and mirrors, must be done for non |
e atoms will absorb light at frequencies or | wavelengths characteristic of the element of interest ( |
a natural autofluorescence at the detection | wavelengths commonly used. |
These pigments have maximal absorbance at | wavelengths corresponding to 350 nm, 440 nm, and 540 nm |
rating in blue to ultraviolet region, where | wavelengths down to 250 nm (far UV) were achieved. |
the shift in wavelength of light to longer | wavelengths due to a speedup - very precisely over time |
een the far infrared and the sub-millimeter | wavelengths, effectively covering wavelengths between t |
The ATM made observations at a variety of | wavelengths, from extreme ultraviolet to infrared. |
es range from about 20 to 250 GHz, covering | wavelengths from microwave to the edge of the terahertz |
ned to take correlated images in a range of | wavelengths from visible light, through the Lyman alpha |
men may be yellow, green, or pale-red, with | wavelengths from 510 to 670 nanometers. |
developed the highest power diode lasers at | wavelengths from 0.8 to 2.7 µm, introducing a new and r |
and short-wave UVA (ultraviolet) rays with | wavelengths from 280 to 320 nm, protecting the skin fro |
Dwingeloo 2 was first detected at radio | wavelengths from the 21 cm emission line of neutral ato |
The material is also highly lambertian at | wavelengths from 257 nm to 10600 nm, although reflectiv |
ich they combined information from multiple | wavelengths from Hubble, ESO's telescope and NASA's Cha |
is designed to measure solar radiation with | wavelengths from 200 nanometers - 100 micrometers. |
At these high frequencies the short | wavelengths give the radiation a very directional quali |
has been observed at a variety of different | wavelengths, giving us different types of information a |
the spectrum but is strongly reflective at | wavelengths greater than 700 nm. |
infrared wavelength of about 860 nm) out to | wavelengths greater than 20 µm; correspondingly, CdTe i |
ht with the same power at longer or shorter | wavelengths has a lower luminous energy. |
often more intense at UHF, because shorter | wavelengths have much greater refraction angles than lo |
recent surveys ranging from radio to X-ray | wavelengths have observed the region to incredible dept |
Employing shorter | wavelengths implied abandoning microscopy and true imag |
he bottom half of the ring is three quarter | wavelengths in length. |
roducts, thermal measurements are taken for | wavelengths in the infrared. |
APEX is designed to work at sub-millimetre | wavelengths, in the 0.2 to 1.5 mm range - between infra |
It has been observed at X-ray | wavelengths in observations using the Chandra and XMM N |
ponse of human or animal tissue to light at | wavelengths in the red and infrared ranges where tissue |
vibrational states excited by very specific | wavelengths in this band, thus the atmospheric gasses s |
At radio | wavelengths, interferometers such as the Very Large Arr |
Typical spectra at these | wavelengths involve rovibrational excitation, i.e., exc |
ht, and the ratio of the emissions at those | wavelengths is directly correlated to the amount of int |
emnant was not seen earlier because in most | wavelengths it is lost in the image of the Vela remnant |
e the T-dwarf fades away towards the longer | wavelengths, it appears quite blue in this image. |
In optical | wavelengths, it has a strong resemblance to Messier 104 |
Far-ultraviolet radiation of | wavelengths less than 200 nm are used to selectively re |
very hot object emit strongly at such short | wavelengths, limiting heat-seeking systems using uncool |
asily visible when its light is filtered to | wavelengths longer than the cutoff value, but will "dro |
s, as it is opaque to infrared radiation of | wavelengths longer than about 2.5 μm. |
In order to avoid this problem much shorter | wavelengths needed to be used, and experiments on the O |
erposition of fringes generated by multiple | wavelengths, obtaining peak fringe contrast as a functi |
ectrons and loss of sharpness in the longer | wavelengths occurs. |
oured filters are used to measure different | wavelengths of light from stars. |
iment they detected an excess brightness at | wavelengths of 0.5 and 0.7 mm. |
The two different | wavelengths of radio waves used permit the altimeter to |
ture cause the crystal to reflect different | wavelengths of light which changes the color of the sto |
only used to detect radiation at only short | wavelengths of less than 2 micrometers. |
cientist, exposed green plants to differing | wavelengths of light, he noticed that at wavelengths of |
The shorter | wavelengths of the X band allow for higher resolution i |
From the perspective of microwaves (with | wavelengths of 12 cm) this screen finishes a Faraday ca |
IF-spectrum according to the amplitude and | wavelengths of the acoustic waves in the crystal. |
plets which are of a comparable size to the | wavelengths of visible light. |
Sun and all sensitive to slightly different | wavelengths of ultraviolet light. |
the cones have maximum absorption values at | wavelengths of about 420 nm (blue), 534 nm (Bluish-Gree |
al microscopic pigments that absorb certain | wavelengths of light and reflect others, creating a vis |
eyes from damage from visible and invisible | wavelengths of laser light. |
However, further analysis of | wavelengths of the emitted light proved that they were |
Many | wavelengths of light, ranging from the ultraviolet to t |
sult of water's selective absorption of red | wavelengths of visible light. |
mpton wavelength, which is just the Compton | wavelengths of the electron and the proton added togeth |
nt absorption spectra, then there may exist | wavelengths of light where σa is high and σb is low. |
ision-the ability to discern four different | wavelengths of light-and thus at least this many (and p |
tput line, Nd:YAG has weaker transitions at | wavelengths of 1052 nm, 1074 nm, 1112 nm, 1319 nm, and |
s particles which are much smaller than the | wavelengths of visible light. |
appear to be limited to a specified set of | wavelengths of laser, and administering LLLT below the |
n at large energies (corresponding to small | wavelengths of the order of the constant length l in th |
surface can be determined by analyzing the | wavelengths of light emitted by the plasma. |
be used to observe astronomical objects at | wavelengths of the electromagnetic spectrum that cannot |
r) to pass only a narrow (<0.1 nm) range of | wavelengths of light centred around the H-alpha emissio |
through the use of 2.3 and 5.5 T fields and | wavelengths of 1064 nm. |
man photoreceptor absorbances for different | wavelengths of light |
icle size distribution forms unusually long | wavelengths of 1-25 m where the wind is not strong enou |
nchromatic" cells that are sensitive to all | wavelengths of visible light and collect a larger amoun |
Some reactants are able to use specific | wavelengths of light more effectively to complete their |
ame part of Sports Service and moved to the | wavelengths of the BBC Third Programme (used for other |
se other molecules are detected using other | wavelengths of light. |
ogy which only been limited to the isolated | wavelengths of HeNe and CO2 lasers and limited number o |
lours used in this image represent specific | wavelengths of infrared light. |
aser gain media have a number of transition | wavelengths on which laser operation can be achieved. |
measurement of the solar irradiance on two | wavelengths, one in a water absorption band, and the ot |
bia, the military wanted radar systems with | wavelengths only a few millimeters. |
cal observations in the millimeter range of | wavelengths, operated by the Institute for Radio Astron |
Each cone type responds best to certain | wavelengths, or colors, of light because each type has |
velength, not producing a broad spectrum of | wavelengths or energies. |
properties to steer light (i.e., to switch | wavelengths or signals within a given fiber). |
In LLLT, red light and some near infra-red | wavelengths penetrate tissue in order to increase cellu |
The | wavelengths produced by most photocytes fall close to 4 |
ake very accurate measurements of the X-ray | wavelengths produced by atoms of different elements. |
International Film Festival as part of the | Wavelengths programming. |
e centimeter band or centimeter wave as the | wavelengths range from ten to one centimeters. |
ar diameter was measured in 1998 at various | wavelengths ranging from 500-850 nm. |
t, and firings of the orbiter's engines, in | wavelengths ranging from infrared to far ultraviolet. |
Visible light, with | wavelengths ranging between 400 nm and 700 nm, passes e |
erty of adding dispersion-namely, different | wavelengths reflected from the grating will be subject |
spectrum graph would show spikes above the | wavelengths representing the colors red and blue. |
the atmosphere is completely opaque to many | wavelengths requiring the use of satellites to make obs |
Since only some | wavelengths resonate within the loop, it functions as a |
lecules tend to absorb radiation at shorter | wavelengths, resulting in a remarkable spectrum with ev |
es associated with energy emission at these | wavelengths, scientists can calculate a variety of surf |
axies in the HUDF that were not detected at | wavelengths shorter than the near-infrared J band, two |
Solar imaging cameras at | wavelengths shorter than 60 A, of focal length 150 mm a |
Although operation on | wavelengths shorter than 200 meters was technically ill |
Microtexture has | wavelengths shorter than 0.5 mm. |
Ultraviolet (UV) detectors work with | wavelengths shorter than 300 nm. |
At | wavelengths shorter than λ0, M(λ) is negative and incre |
, it outputs multiple beams over a range of | wavelengths simultaneously. |
material for both infrared and ultraviolet | wavelengths, since it is transparent in these regions ( |
ly easy to use electrons or neutrons having | wavelengths smaller than a nanometer, electrons and neu |
Discs utilizing very short | wavelengths such as UV or X-rays. |
requires the use of radiation with shorter | wavelengths, such as X-rays or neutrons beam. |
ke lasers to reflect a wider range of light | wavelengths than ordinary dielectric mirrors, or to com |
nded the range of IR measurements to longer | wavelengths than had ever been reached. |
Allophycocyanin absorbs and emits at longer | wavelengths than Phycocyanin C or Phycocyanin R. Phycoc |
to incandescence and emit light at shorter | wavelengths than would be expected for a typical blackb |
X-ray telescope, shorter | wavelengths than ultraviolet light |
It passes | wavelengths that are a multiple of the cavity's resonan |
analyte atoms emit light at characteristic | wavelengths that can be dispersed with a monochromator |
There are | wavelengths that people cannot see, there are sounds th |
However for | wavelengths that approximate those for which the atom s |
pectrum of the microcavity, a long range of | wavelengths, that is reflected and a single one being t |
rbing red, orange, yellow, and green light, | wavelengths that are not well absorbed by chlorophyll a |
light by retina pigments corresponds to the | wavelengths that best activate photoreceptor cells, thi |
it of the Lyman series of the spectrum with | wavelengths that are shorter than 91.1267 nanometres an |
rs where the name of the filter denotes the | wavelengths that are blocked, and in line with the conv |
ctually the sum of many colors of different | wavelengths, the light of knowledge of our world is com |
capabilities of the SST because at visible | wavelengths the stars are completely obscured by inters |
hen simultaneously exposed to light of both | wavelengths the rate of photosynthesis increases. |
At GHz | wavelengths, the skin depth is less than the thickness |
At shorter | wavelengths the CIB level could not be correctly determ |
s differ by a whole number (including 0) of | wavelengths, there is constructive interference and a s |
specifically with respect to which visible | wavelengths they absorb and how much. |
and allows images to be taken at different | wavelengths to be compared. |
-oximeter measures absorption at additional | wavelengths to distinguish CO from O2 and determines th |
d, it will make observations in ultraviolet | wavelengths to measure the history of star formation in |
scopic data at optical, infrared, and radio | wavelengths to try to formulate a coherent picture of t |
rather delicate balance, since the shorter | wavelengths travel a larger distance through air. |
g in the stretched pulse, because different | wavelengths travel at different speeds in the dispersiv |
This means that longer | wavelengths travel faster through these materials. |
mples containing species which interfere at | wavelengths typically used for the analyte. |
Despite being opaque at visible-light | wavelengths, use of the Very Large Telescope at Cerro P |
ute to anomalous scattering at normal X-ray | wavelengths used for X-ray crystallography . |
of the sky and experimented with different | wavelengths using various photographic filters and mana |
A comparison of images taken at different | wavelengths was done using low-intermediate-resolution |
larly important for observing at millimeter | wavelengths, where incoming signals can be absorbed by |
e, and therefore is normally not favored at | wavelengths where these techniques can be applied. |
ted with light of a specific wavelength (or | wavelengths) which is absorbed by the fluorophores, cau |
lated to be about 35th magnitude at visible | wavelengths, which is undetectable. |
tron moderators cool the neutrons to useful | wavelengths, which are then directed at a suite of inst |
cles prevents the transmittance of infrared | wavelengths while still allowing the transmittance of v |
Irradiation at these | wavelengths will provide photostationary states that co |
Therefore different | wavelengths will travel down an optical fiber at differ |
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