「detector」の共起表現(1語左で並び替え)3ページ目

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one super-module of the Projectile Spectator	Detector (a calorimeter) was installed downstream of t
In the 1970s he invented the SPRITE	detector (Signal PRocessing In The Element) which was
is detected with a wide-bandwidth square-low	detector the intensity noise will be converted into cu
als, something that the coherer (the standard	detector of the time) could not do.
t to be fitted with the ASDIC (Anti Submarine	Detector Investigation Committee) underwater sensor sy
ctron microscopes, even though the first such	detector was made available as early as 1956.
ling was to expand the seeker's lead sulphide	detector element's sensitivity range to longer wavelen
photomultiplier tubes in the Super-Kamiokande	detector imploded, apparently in a chain reaction as t
spectrometers enabled by the superconducting	detector arrays.
The SuperNEMO	detector will consist of 20 modules each containing ap
DAPHNE is a cylinder symmetric	detector that was built to detect mainly charged parti
s to the group of people working on the TASSO	detector, at PETRA, at DESY.
rically cooled MCT (Mercury Cadmium Telluride	detector).
ich case the (nearly) steady component of the	detector output is a good measure of the instantaneous
of a defined energy are backscattered to the	detector if they collide with an atomic nucleus.
The	detector end of a simple x-ray diffractometer with an
ved signal to a level sufficient to drive the	detector stage.
ctive interference and a strong signal at the	detector.
The bubble development in the	detector is accompanied by an acoustic shock wave that
order to filter out the common events so the	detector is not overwhelmed, the electrons must pass t
system focuses the thermal radiation onto the	detector.
, if no higher energy particles penetrate the	detector walls, the SST-Foil should only measure elect
e overall signal production efficiency of the	detector, however, also depends on the quantum efficie
Roughly spherical, the	detector measures 30 feet across.
Since the ray cones approaching the	detector surface have the same angle of incidence and
by the linear stage and appear finally to the	detector as if it were a sideband of the carrier, it i
The outermost layer of the	detector detects muons.
er signal is given when the sample enters the	detector because the oxidized carbons are not ionized
be very low and a radio receiver used as the	detector.
a meter to display the output from the	detector
s VD slowly recovers to Va, and therefore the	detector is ready to be ignited again.
th a so-called makeup gas flowing through the	detector chamber.
d by this low voltage and will only reach the	detector if their direction of travel takes them to it
The	detector CCD is 2k X 2k with a 15 micrometer pixel siz
The	detector aims at measurement of total cross section, e
sufficient energy such that it arrives at the	detector at the same time as the red ion.
ic current, which is the signal output of the	detector.
ill then drift through the flight tube to the	detector in the same time.
The	detector is operated in consortium with several univer
The	detector sensitivity can be adjusted by changing the t
the satellite made the interpretation of the	detector data very difficult.
ewly polarized photon will be measured at the	detector.
of high energy and pass straight through the	detector.
The scattered gamma rays reaching the	detector, at the fixed station from the source, are co
The order of migration seen by the	detector is shown in figure 3: small multiply charged
ting the spatial information contained in the	detector signal we can more accurately localize the γ-
The	detector turned on in May 1999, and was turned off on
The first part of NT-200, the	detector NT-36 with 36 optical modules (OMs) at 3 shor
/z but different kinetic energy arrive at the	detector at the same time.
gain is how the amount of signal given by the	detector varies as a function of the amount of light (
As a charged particle travels through the	detector, it ionizes the gas between the plates.
rent is the amount of signal given out by the	detector when there is no incident light (hence dark f
In a second phase (end of 2007), the	detector is planned to be moved underground.
rcentage of the fluorescence picked up by the	detector is also dependent upon the system.
The	detector spins with the spacecraft on a plane containi
sed for fine adjustment of the sample and the	detector positions.
On passing through the	detector gas, a particle will produce primary ionizati
The	detector is positioned to be centered to the light ray
ticles but they live long enough to leave the	detector.
s of dust between the gamma-ray burst and the	detector.
The use of a mass spectrometer as the	detector in gas chromatography was developed during th
The name of the	detector is a playful pun, which was bestowed upon it
a fraction of its energy is registered by the	detector.
uded new superconducting quadrupoles near the	detector.
The	detector is built of 10 planes with 20 paddles each.
aser intensity, the quantum efficiency of the	detector and the full scattering volume and solid angl
tter) between the point of reflection and the	detector.
photons produced by the PID lamp used in the	detector.
es are necessary: an underground site for the	detector, to limit the effect of the seismic noise, an
Deployment and connection of the	detector are performed in cooperation with the French
The	detector was commissioned in the early 90's, and was d
By contrast, if the	detector sees photons emitted directly from a glowing
era phones, because the low resolution of the	detector allows a loose focusing on the CCD without no
can undergo a phase transition at a time, the	detector can stay active for much longer periods than
flicker frequency of a fire (1 to 20 Hz) the	detector is made less sensitive to false alarms, cause
of SSNTDs is that charged particles break the	detector within nanometers down the path in such a way
y, inexpensive and hearty construction of the	detector.
etween a broad spectrum photon source and the	detector.
hydrogen is consumed which is recorded by the	detector.
ition of endcaps of similar construction, the	detector covered 98% of the solid angle around the int
After its decommissioning at SLAC, the	detector was carried to DESY, where it was used for b-
The	detector converts RF signals directly to information,
The	detector is able to measure charged particles in the e
The	detector was partially restored by redistributing the
o discriminate against particles entering the	detector from below.
upersymmetric particle, LSP (which leaves the	detector unseen).
The	detector consists primarily of a scintillator inside a
and positron created were measured within the	detector volume,and the axis of the V of the two emerg
The intensity of the light hitting the	detector depends on the relative positions of the two
ich the infrared scene was scanned across the	detector (made from HgCdTe) at the same rate as the ca
The	detector consists of a special center-tapped transform
ten built underground in order to isolate the	detector from cosmic rays and other background radiati
is nearing the levels where theoretically the	detector should start to detect dark matter.
The	detector is a photodiode made of a 1.2 kg germanium cr
25 (GX5-1), but the spatial resolution of the	detector was insufficient to resolve Sgr X-5 from the
Even though the	detector operated only during a few months in the summ
Case described the	detector material as consisting of thallium, oxygen an
between length of DNA strand and time at the	detector.
The LEGRI system included the	Detector Unit, Mask Unit, Power Supply, Digital Proces
eld that the ions recombine after passing the	detector to reform their original molecules, however o
Specify the	detector geometry.
The polarized radiation focused onto the	detector is doubly modulated, both by the PEM and by t
oherent superposition of emitted light on the	detector is possible.
These two components interfere in the	detector and produce signals, which permit the detecti
ation of intensity from any Debye cone at the	detector provides order(s) of magnitude increase in in
band of light initially traveling toward the	detector, has been effectively scattered in other dire
The	detector was sensitive to 0.5-2.0
The	detector has a sensitive receiver tuned for these harm
ating and thus have the longest tracks in the	detector.
Otherwise the	detector might be damaged.
The output signal of the	detector (Temperature T) is related to the thermal rad
The	detector system was built in 1990.
observe the photon is done after it hits the	detector.
of charged particles traveling through their	detector.
A Leslie cube (left) and a thermal	detector (right)
he cube is filled with hot water, the thermal	detector (on the far right in the figure), shows much
In units using these	detector arrays, the intensities of all wavelengths (w
A research group at GSI is named after this	detector.
This	detector allows for immediate determination of the mol
In this circumstance the fixed threshold	detector would probably be best.
A solid-state nuclear track	detector or SSNTD (also known as an etched track detec
See also solid state nuclear track	detector.
eing used extensively in the central tracking	detector of the D0 experiment, and for muon cooling st
A Pulse transition	detector is used in flip flops in order to achieve edg
"Oscillation Responsive Device" (vacuum tube	detector - no grid), filed May 1906, issued November 1
1969, Australian Customs Service had only two	detector dogs.
The UA2	detector
USS	Detector (AMc-75) was an Accentor-class coastal minesw
h performance liquid chromatography with a UV	detector or by LC-MS.
repair light sets: Quick Fix Trigger, Voltage	Detector, and/or Bulb & Fuse Tester.
The Large Volume	Detector (LVD) is a particle physics experiment situat
Д, НЕйтринный ВОдный Детектор, Neutrino Water	Detector) is a neutrino detector and cosmic ray experi
AIGO is the only gravitational wave	detector within the Southern Hemisphere.
The laser interferometric gravitational wave	detector is so named because it is to be most sensitiv
An interferometric gravitational wave	detector is a gravitational wave detector that uses la
The Mario Schenberg (Gravitational Wave	Detector, Antenna, or Brazilian Graviton Project) is a
A) is a novel scheme for a gravitational wave	detector, proposed by M. Ando, et.
ogenic resonant Weber bar, gravitational wave	detector run by Warren Johnson, et.
opment for the space-borne gravitational wave	detector LISA (Laser Interferometer Space Antenna), an
a future third generation gravitational wave	detector, currently being designed by different instit
GEO600 near Sarstedt, Germany, and LIGO, with	detector facilities in Hanford, Washington, and Living
y be readily detected the plug is coated with	detector paint.
SPACEHAB Payloads include the Advanced X-Ray	Detector (ADV XDT), the Advanced Commercial Generic Bi
On board is a hard X-ray	detector (27-189 keV) with a 5.1 cm2 NaI(Tl) scintilla
Development of a novel X-ray	detector technique for use in medical imaging;
The Vela 5B satellite X-ray	detector remained functional for over ten years.
The scintillation X-ray	detector (XC) aboard Vela 5A and its twin Vela 5B cons
red with the University of Utrecht hard X-ray	detector with a time resolution of 1.2 s (< 100 keV) a
The small area of the X-ray	detector, thick Mylar window counters, and high scan r
one sounding rocket flight carrying an X-ray	detector flown on many flights that yields trustworthy
the Naval Research Laboratory loaded an X-ray	detector on board an Aerobee that is launched from the

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