「Infra-red」の共起表現一覧(1語右で並び替え)
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Samarium(III) oxide is used in optical and | infrared absorbing glass to absorb infrared radiation. |
rational motions, which are measureable in an | infrared absorption spectrum. |
wn to have a monoclinic C2/m symmetry and its | infrared absorption behaviour was attributed to the as |
ng: it exhibits a dark-red color, very strong | infrared absorption, and a magnetic collapse. |
The satellite observes in the | infrared, allowing for better observation towards the |
(PRocess Exploration through Measurements of | Infrared and millimetre-wave Emitted Radiation) |
trating on theoretical astronomy and optical, | infrared and x-ray observations |
data for organic compounds including that for | infrared and NMR spectroscopy and mass spectrometry. |
the band in 1996 they reformed under the name | Infrared and recorded a demo before disbanding in 1997 |
on remote sensing equipment for visible, near | infrared, and soft and hard X-ray frequencies. |
It has | infrared and stereo sound sensors on its head, and tou |
have included visible light imaging systems, | infrared and ultraviolet spectrometers, and an ultrast |
ceeded in finding German specialists, e.g. in | infrared and wireless Pathfinding and engaged them to |
s capable of capturing images in the visible, | infrared, and water vapor regions of the electromagnet |
work involved solar spectroscopy in the near | infrared and participation in a solar flare patrol pro |
have a wide transparency range from UV to the | infrared and therefore had been used for cuvettes, pri |
SS photometric system, I and V represent near | infrared and visual, respectively. |
will provide observation data between the far | infrared and the sub-millimeter wavelengths, effective |
a part of the spectrum between microwaves and | infrared, and the traditional bounds of electronics, a |
be shown that overtones are forbidden in both | infrared and Raman spectra. |
h as an electric soldering iron, cold blades, | infrared, and lasers. |
Reinhard Genzel studies | infrared- and submillimetre astronomy. |
Infrared and ultraviolet are also greatly blocked. | |
Infrared and Raman Spectra of Polyatomic Molecules. | |
th imaging and spectroscopic data at optical, | infrared, and radio wavelengths to try to formulate a |
very quickly during the evolution towards the | infrared, and thus the flow effectively collapses on a |
Optical, | infrared, and X-ray observations taken by the Hubble S |
s commonly used as a window material for both | infrared and ultraviolet wavelengths, since it is tran |
one of the world's highest sites for optical, | infrared and gamma-ray telescopes. |
st laser methods are also now possible in the | infrared and visible spectral regions. |
e viewer gets to hear more news reports about | infrared and night vision technology and laser-guided |
Infrared and Raman Studies of Skin and Hair: A review | |
nger wavelengths (X-ray, ultraviolet, visual, | infrared, and radio). |
ro-optical fire control system with 27x zoom, | infrared and low-light modes, a laser rangefinder, and |
ger wavelengths (X-ray, ultraviolet, optical, | infrared, and radio). |
It can also be seen in | infrared and is a weak radio source. |
heavy-ion tracks in lunar samples, as well as | infrared and UV spectra of interstellar dust. |
s has been one of Europe's leading figures in | infrared and submillimetre astronomy, and observationa |
Rotational transitions take place in the far | infrared and microwave regions. |
This covers near-ultraviolet, visible and | infrared areas of the spectrum. |
the three asteroids discovered with data from | Infrared Astronomical Satellite in 1983, and was named |
e comet was named after its discoverers - the | Infrared Astronomical Satellite and two amateur astron |
The | Infrared Astronomical Satellite (IRAS) was the first-e |
tar's name comes from the 1983 survey mission | Infrared Astronomical Satellite (IRAS). |
e it the second best location for optical and | infrared astronomy in the Northern Hemisphere, after M |
The development of radio astronomy, | infrared astronomy and submillimeter astronomy in the |
orne telescope, Stratospheric Observatory for | Infrared Astronomy (SOFIA), completed its first test f |
AKARI, in astronomy, is an | infrared astronomy satellite developed by JAXA, in coo |
hysicist who works primarily in the fields of | infrared astronomy instrumention and adaptive optics. |
ientist for the Stratospheric Observatory for | Infrared Astronomy (SOFIA), which is a 2.7m infrared t |
His scientific work on | Infrared astronomy as a professor at Cornell Universit |
ntegral part of Stratospheric Observatory for | Infrared Astronomy (SOFIA). |
CIBER was an | infrared astronomy mission launched from White Sands a |
SOFIA (Stratospheric Observatory for | infrared Astronomy) - NASA 747SP |
erstellar medium, globular cluster formation, | infrared astronomy, and near-Earth objects. |
particle physics, solar physics, the planets, | infrared astronomy, and millimeter- and submillimeter- |
19-28 (PDF), (from "IV National Conference on | Infrared Astronomy, in honour of Paolo Maffei", Perugi |
Robinson's largest contributions have been in | infrared astronomy, he was able to use data from IRAS |
In | infrared astronomy, the M band refers to an atmospheri |
recognized for his expertise and research in | infrared astronomy. |
ializing in astrophysical instrumentation and | infrared astronomy. |
rvatory and the Stratospheric Observatory for | Infrared Astronomy. |
ializing in astrophysical instrumentation and | infrared astronomy. |
adiative transfer model for the CNES/EUMETSAT | Infrared Atmospheric Sounder Interferometer (IASI) lev |
rface brightness was identified as the cosmic | infrared background at 60, 100, 140 and 240μm. |
antially greater sensitivity in the 10-100 μm | infrared band (IR band); the telescope is intended to |
and must be studied in the X-ray, radio, and | infrared bands. |
amera to the Wii and put it near to the Wii's | infrared bar. |
se firefighter movement and others utilize an | infrared beam against a mirror mounted on a spring. |
the concentrations of respired gases using an | infrared beam of light. |
transmitted to the climber using a high-power | infrared beam. |
of transmitted energy such as radar waves or | infrared beams to detect vehicles passing over the roa |
In modern open field apparatus | infrared beams can be used to automate the assessment |
s are used in people counter devices, such as | infrared beams, computer vision, thermal imaging and p |
Uses modulating | infrared burner that is triggered by water-flow or the |
It was replaced by the Near | Infrared Camera and Multi-Object Spectrometer (NICMOS) |
The Near | Infrared Camera and Multi-Object Spectrometer (NICMOS) |
pe supports a 1024x1024 HAWAII-1 based HgCdTe | infrared camera operating between 0.8 and 2.5 µm. |
Shuttle Lee-side Temperature Sensing (SILTS) | infrared camera package made its second flight aboard |
OWL: a hyperspectral thermal | infrared camera developed by Specim . |
His team also developed the first color | infrared camera for Kitt Peak National Observatory in |
in link and barbed wire fences with light and | infrared camera poles. |
The Near | Infrared Camera for the Keck I telescope is so sensiti |
cone is jettisoned to allow a high resolution | infrared camera to observe the target area (the bunt e |
amera for Surveys (ACS) and possibly the Near | Infrared Camera and Multi-Object Spectrometer (NICMOS) |
s sensitive Si-based bolometers (see uncooled | infrared camera), InSb and photon-counting superconduc |
together with electronics and optics to make | infrared cameras for thermography. |
or scientific observation that proved through | infrared cameras she was originally wearing a bonnet a |
hey have state-of-the-art imaging systems and | infrared cameras and provide a global scan every two d |
LLLTVs tend to be more affordable than | infrared cameras, which typically cover ranges from 3 |
Main article: | Infrared cleaning |
The Hipparcos satellite and | infrared color-magnitude diagram fitting have been use |
The Hipparcos satellite and | infrared color-magnitude diagram fitting have been use |
Two-Micron Sky Survey, or IRc, or | Infrared compact, or Caltech infrared catalog is the a |
ntire range-from vacuum tube, solid state and | infrared components, to laser and fiber optic technolo |
tly becomes extremely hot and radiates in the | infrared, concentrating the heating of oil for popcorn |
Circular | infrared connection point for Canon's Barcode Reader |
Additionally the HP-40G does not have | infrared connectivity, and is limited to 27 variables. |
Infrared cooking differs from other forms of grilling, | |
"IR filter" still can be used as a synonym of | infrared cut-off filter. |
telescope at Kitt Peak National Observatory; | infrared data from the Spitzer Space Telescope. |
ects two types of data, hyperspectral thermal | infrared data from 6 to 50 micrometers (μm) and bolome |
ge was taken on 28 November 2006 by the UKIRT | Infrared Deep Sky Survey (UKIDSS) with a recovery imag |
electron tunnel sensors for acceleration and | infrared detection and initiated the NASA/JPL microins |
egradation as well as methods to characterize | infrared detection and display systems. |
tocopying (xerography); lead sulfide, used in | infrared detection applications, such as the U.S. Side |
ion, radar detection, acoustic detection, and | infrared detection. |
owave propagation in free electron media, and | infrared detection. |
IR5 MCT: | infrared detector for highly demanding applications in |
in the fields of narrow gap semiconductor and | infrared detector research. |
e (Co 2TR) Through Barrier Materials Using An | Infrared Detector |
wth of mercury cadmium telluride (HgCdTe), an | infrared detector material. |
make lead tin telluride, which is used as an | infrared detector material. |
make lead tin telluride, which is used as an | infrared detector material. |
An | infrared detector is a photodetector that reacts to in |
and NOAO to develop the world's largest InSb | infrared detector array (the first megapixel device wi |
Infrared Detectors and Emitters: Materials and Devices | |
Infrared detectors on the Spitzer Space Telescope can | |
rk culminated in the development of long wave | infrared detectors used during the second world war. |
Mercury zinc telluride is used in | infrared detectors and arrays for infrared imaging and |
They are used as | infrared detectors or thermoelectrics. |
on the sky, the image plane has 16 arrays of | infrared detectors, each array with 2048x2048 pixels o |
By having multiple | infrared detectors, each sensing a particular waveleng |
ed into an articulator (registration based on | infrared devices) |
The | Infrared Diamond Lure defense is put into effect. |
e color, high-resolution black and white, and | infrared digital cameras atop telescoping arms. |
o-mass particles in the cycle of the diagram ( | infrared divergence) or due to insufficient falloff of |
vation for developing SCET was to control the | infrared divergences that occur in QCD calculations th |
These images are available in the visible and | infrared domains. |
Reflection-absorption | infrared, dual polarisation interferometry, surface en |
sion which was unexpected as the extrapolated | infrared dust signal to microwave frequencies should h |
Recently, | infrared echo of Cassiopeia A explosion was observed o |
CRISM measures visible and | infrared electromagnetic radiation from 370 to 3920 na |
rument on the Spitzer Space Telescope, excess | infrared emission has been observed from the star, whi |
This system displays an excess of | infrared emission, which may indicate the presence of |
kinematical peculiarities, nuclear radio and | infrared emission, and starburst or active galactic nu |
discovered by Paolo Maffei in 1968 from their | infrared emission. |
ound main sequence stars through their excess | infrared emission. |
d the neighboring Maffei 2 in 1968 from their | infrared emissions. |
nts would literally be 'blinded' by their own | infrared emissions. |
greatest difference is probably in their near | infrared emissions. |
, SWout or reflected solar radiation, LWin or | infrared emitted by the sky and LWout or infrared emit |
By knowing the amount of | infrared energy emitted by the object and its emissivi |
Spitzer Space Telescope failed to detect any | infrared excess at 70 micrometres or at 24 micrometres |
Denebola shows a strong | infrared excess, which means there must be a debris di |
The Near Field | Infrared Experiment (NFIRE) is a satellite which was p |
SMINE: Japan Astrometry Satellite Mission for | INfrared Exploration) is a 35 kg astrometric microsate |
Variations in the thermal | infrared false-color image are due to differences in t |
an anti-halation layer in Kodak's High Speed | Infrared film (HIE) is the cause of the ethereal "glow |
be used because "winding problems may occur"; | infrared film is not recommended because the frame cou |
Kodak High-Speed | Infrared film, also known as Kodak HIE was a popular b |
Sigma has also revised the | infrared filter (dust protector); it is now a round sn |
(5 elements, glass lenses plus | infrared filter), like 48mm for 35mm film |
Infrared filters are readily available at low cost fro | |
and green filters, later switched to red and | infrared filters. |
ific research into the Earth's magnetosphere, | infrared flux and ultraviolet flux. |
ory carried out an experiments to measure the | infrared flux during the eclipse, due to the cloud som |
ink and Low Altitude Navigation and Targeting | Infrared for Night (LANTIRN). |
Infrared Fourier Spectrometer | |
It is an | infrared Fourier Transform spectrometer and provides k |
terious ring around SGR 1900+14 at two narrow | infrared frequencies in 2005 and 2007. |
in experiments with the Shiva laser that the | infrared frequencies generated by the laser lost most |
crowave radiation is between common radio and | infrared frequencies. |
Bulk CdTe is transparent in the | infrared, from close to its band gap energy (1.44 eV a |
on furnace, belt furnace, atmosphere furnace, | infrared furnace and fast fire furnace, to just list a |
It is one of the most ultraluminous | infrared galaxies with power derived from an accreting |
chanisms of the formation of (Ultra-)Luminous | Infrared Galaxies ((U)LIRGs), as it provides data on t |
omical objects, like quasars or ultraluminous | infrared galaxies, which are very bright in the infrar |
he most common principles for CO2 sensors are | infrared gas sensors (NDIR) and chemical gas sensors. |
Barugon approaches the boat carrying the | infrared generator and destroys it. |
Gilbert A. Esquerdo and John C. Barentine in | infrared give rise to suspects that it has the Hubble |
Grilling enthusiasts claim food cooked on an | infrared grill tastes similar to food from char-grills |
Also, | infrared grills have the advantages of instant ignitio |
Proponents say that food cooked on | infrared grills seems juicier. |
The | infrared group built the NICMOS instrument for the Hub |
ially for US Navy, uses a modified Maverick D | infrared guidance system optimized for tracking ships |
The prototypes were fitted with | infrared guidance systems from GAR-2A/B (AIM-4C/D) Fal |
g for terrestrial planets in the optical/near | infrared has the advantage that the diffraction limit |
es with multiple telescopes, operating in the | infrared, have imaged and confirmed this phenomenon. |
Visitors are given | infrared headphones in order to listen to almost 200 m |
heoretical models he developed to visible and | infrared Hubble data collected by then Harvard graduat |
The reddish colors in the false-colour | infrared image suggest the distribution of hydrocarbon |
Infrared image of 2M1207 (blueish) and 2M1207b (reddis | |
THEMIS: a multispectral thermal | infrared imager on board the 2001 Mars Odyssey spacecr |
The Meteosat Visible and | Infrared Imager (or MVIRI) is the scientific instrumen |
There is also an | infrared imager, but it is often "borrowed" by astrono |
ery permits the most detailed imagery whereas | infrared imagery has the advantage of availability at |
They also reported that animated | infrared imagery had shown that deep convection was fl |
Infrared images of the Trapezium are better able to pe | |
t more recently they've been found on Mars in | infrared images taken from orbit by Mars Odyssey's the |
ispectral imager to capture visible light and | infrared images of the continental United States, a so |
Infrared images from instruments mounted on the telesc | |
They said that in | infrared images the bright, western part resembles a d |
The primary focus of Becklin's research is | infrared imaging and spectroscopy, including the searc |
having just completed the construction of an | infrared imaging spectrograph, Mimir, in collaboration |
eved in March 2009 in the visible region, and | infrared imaging underway as of June 2009, the observa |
rmography (FMT) is a microscopy technique for | infrared imaging of temperature distribution in small |
at the University of Florida, specializing in | Infrared imaging, took numerous infrared photographs o |
ype of microwave radiation that is closest to | infrared in the light spectrum. |
n such as gamma rays, X-rays, ultraviolet and | infrared, in addition to visible light. |
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