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1 ins deterministically via a modified Franson interferometer.
2 r with a nearly shot-noise limited microwave interferometer.
3 e passes of the e/4 quasiparticle around the interferometer.
4 from two longitudinal locations with a laser interferometer.
5 vidual atoms are detected using a novel atom interferometer.
6 that can be used as a terahertz Mach-Zehnder interferometer.
7 sitive gerbil cochlea using a scanning laser interferometer.
8 in terms of Fabry-Perot modes in an electron interferometer.
9 cochlea using a displacement-sensitive laser interferometer.
10 a magnetic field sensor based on a spin wave interferometer.
11 brid (SOH) slot waveguide based Mach-Zehnder interferometer.
12 smear statistical photon bunching in the HOM interferometer.
13 he repeatability of a commercially available interferometer.
14 ven after the photon has already entered the interferometer.
15  the enabler of non-classical dynamics in an interferometer.
16  using a conventional x-ray tube and grating interferometer.
17 turn in living gerbil cochleae using a laser interferometer.
18  the bR adlayer over one or both arms of the interferometer.
19 iliary motions with a dual-beam differential interferometer.
20 background, or later with direct space-based interferometers.
21 year could be detected by gravitational wave interferometers.
22 eters, superconducting gravimeters, and atom interferometers.
23 enhancing the sensitivity of molecular-scale interferometers.
24 s, such as common- and double path waveguide interferometers.
25 ase contrast than current near-field grating interferometers.
26 ent, most sensitive methods based on crystal interferometers.
27 GO) film is deposited on a fiber-optic modal interferometer, acting as both the fluorescent quencher
28 sured with a radial shearing speckle pattern interferometer after an increase in intraocular pressure
29 icroscopic examination of the fundus, an OCT interferometer, an OCT beam delivery system designed for
30 ter Gravitational-Wave Observatory and Virgo Interferometers, an associated optical transient, SSS17a
31 specialized imaging system, combining Sagnac interferometer and CCD camera images to reconstruct spec
32 spectrometer assembly, employing a step-scan interferometer and focal plane array detector, is analyz
33 d neutrons through a perfect silicon crystal interferometer and perform weak measurements to probe th
34  conditional quantum gates in a Mach-Zehnder interferometer and report a proof-of-principle experimen
35 y comb to self-reference a Ramsey-Borde atom interferometer and synchronize an oscillator at a subhar
36                         Using a Mach-Zehnder interferometer and time-delayed femtosecond laser pulses
37 ny components, such as waveguides, couplers, interferometers and modulators, could be directly integr
38 mple, quantum point contacts (QPC), electron interferometers and quantum dots.
39                  Photonic circuits including interferometers and resonators have been transferred ont
40 rinciples underlying future planet-searching interferometers, and our laboratory instrument will serv
41                                        These interferometers are widely used for precision measuremen
42 cted from an integrated optical Mach-Zehnder interferometer as a passive structure, covered by a bact
43 n electronically reconfigurable Mach-Zehnder interferometer as the frequency reference to reduce the
44 c frequency (CF) tones were measured with an interferometer at up to 15 locations across the basilar
45          Here we report a far-field, two-arm interferometer based on the new nanometric phase grating
46                               A differential interferometer-based microcantilever sensor was develope
47 ed signal to a short XRL amplifier and as an interferometer beam to measure two-dimensional local gai
48 We report here the application of a photonic interferometer biosensor based on a bimodal waveguide (B
49          Integrated planar optical waveguide interferometer biosensors are advantageous combinations
50 es about integrated planar optical waveguide interferometer biosensors can mostly be found in the lit
51 l interferograms, namely IAW, obtained on PS interferometer by subtraction (wavelength by wavelength)
52                                          The interferometer consists of two 45-nm-thick silicon layer
53 o by passing single photons through a Sagnac interferometer containing both a metamaterial with a neg
54    Here we describe the Degree Angular Scale Interferometer (DASI), an array of radio telescopes, whi
55 ion of the CMB with the Degree Angular Scale Interferometer (DASI).
56                     Here we present an X-ray interferometer design that is practical for adaptation t
57          Here we use a small-area edge state interferometer designed to observe quasiparticle interfe
58 tic vibrometer based on a modified Michelson interferometer, designed to serve as a middle-ear microp
59 tional-Wave Observatory (LIGO) and the Virgo interferometer detected gravitational waves (GWs) emanat
60 n integrated device containing three coupled interferometers, eight spatial modes and many classical
61                           We demonstrate the interferometer for a graphene-type hexagonal optical lat
62 ailor and co-workers (1997) on the use of PS interferometer for biosensing, and lowers of 4 orders of
63 ential limitations of the use of porous SiO2 interferometers for quantitative determination of protei
64 developed arrayed nanostructured Fabry-Perot interferometer (FPI) microchips.
65 twin extreme UV pulses to create a molecular interferometer from direct and sequential two-photon ion
66 ing blocks, which permit composing arbitrary interferometer geometries in a digital manner.
67 ll soon be observed and studied by the Laser Interferometer Gravitational Wave Observatory and its in
68                 On 17 August 2017, the Laser Interferometer Gravitational-Wave Observatory (LIGO) and
69 of gravitational waves by the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) det
70 vitational wave source GW170817 by the Laser Interferometer Gravitational-Wave Observatory and Virgo
71 -mass binary black hole mergers by the Laser Interferometer Gravitational-wave Observatory opened the
72                                Our prototype interferometer, having just under one millimetre of base
73 he present experiment using a scanning-laser interferometer, I detected forward-traveling but not bac
74 ing instrument to be implemented on the Keck interferometer in 2001.
75  and simultaneously with a modified spectral interferometer in 30 healthy subjects with two different
76 r, self-aligned, amplitude-division electron interferometer in a conventional transmission electron m
77 ere we used a high-precision, GHz-ultrasonic interferometer in conjunction with a newly developed opt
78 thod by using a thermal-stabilized reference interferometer in conjunction with an ultrahigh-Q microc
79                  Here we study a new type of interferometer in which the beam splitting and recombina
80 be overcome by using a dual-aperture stellar interferometer in which the starlight is cancelled, or '
81 tes are vital to exploring gravity with atom interferometers in greater detail.
82 FT-IR microimaging employing continuous scan interferometers in which the advantages of fast image co
83 a semiconductor laser using a laser-feedback interferometer, in which the terminal voltage of the las
84 the space of Laguerre-Gaussian modes, and an interferometer incorporating such a 'delay' obtains moda
85                                          The interferometer is constructed from a sequence of discret
86                                         This interferometer is fabricated from a single-crystal silic
87                                       As the interferometer is naturally operated at cryogenic temper
88                               A Mach-Zehnder interferometer is used for the homodyne detection.
89            An important advantage of our MCF interferometers is their capability to operate at very h
90  in twenty Asian subjects (20 eyes) using an interferometer (LipiView(R) ocular surface interferomete
91      We report the use of in-line incoherent interferometers made from uniaxial birefringent alpha-ba
92 significance of LLT changes measured by this interferometer may be better interpreted.
93 ation of radio frequency time-of-arrival and interferometer measurements, we observed a sequence of l
94 The detector is based on a tunable microwave interferometer (MIM) with a vector network analyzer (VNA
95            Here, we present the Mach-Zehnder interferometer-miRNA detection system capable of detecti
96 of mid-infrared (MIR; 3-12 mum) Mach-Zehnder interferometers (MZIs).
97                   Using a cesium matter-wave interferometer near a spherical mass in an ultrahigh-vac
98 ed using a direct measurement (by an optical interferometer) of its changes in diameter as it pulsate
99  refractometric detection using the Rayleigh interferometer offers a key advantage for providing accu
100 system and the incorporation of the Rayleigh interferometer onto the ultracentrifuge that had the gre
101 different waves and form new types of hybrid interferometers, opening a door for many applications in
102                            Current bench-top interferometers operate in the near field with limitatio
103 rgeted in the current literature) using a PS interferometer operating in label-free mode without any
104                      Here we present an atom interferometer operating with single trapped atoms, wher
105  modulation (for example, using Mach-Zehnder interferometers or ring resonators).
106 tors use nonreciprocal phase shift (NRPS) in interferometers or ring resonators, but to date NRPS req
107 a recently proposed nanoparticle matter-wave interferometer, originally conceived for tests of the qu
108 maging, it enables a polychromatic far-field interferometer (PFI) without absorption gratings.
109 ce model, encompassing the description of an interferometer phase probed with relevant quantum states
110 e technique for shot noise suppression, this interferometer promises further improvement in sensitivi
111                                          The interferometer provided maps 300 kilometers by 1000 kilo
112       It makes use of the fact that an X-ray interferometer provides a conventional absorption as wel
113 -polariton condensate and employ a Michelson interferometer setup to characterize the short- and long
114 onalized prGO film coated on the fiber-optic interferometer shows high sensitivities for the detectio
115  been enabled by the introduction of grating interferometers so far.
116 re derived from Atmospheric Emitted Radiance Interferometer spectra together with ancillary measureme
117 n interferometer (LipiView(R) ocular surface interferometer, TearScience Inc, Morrisville, NC).
118 , chip-based implementation of a double-beam interferometer that can separate biomolecules based on s
119 mentum space, in analogy to an Aharonov-Bohm interferometer that measures magnetic flux in real space
120                 Here we use a scanning laser interferometer to determine the volume displacement and
121                         We realize an atomic interferometer to measure Berry flux in momentum space,
122                   We have used a laser-diode interferometer to measure in vivo the distribution along
123 -to-noise ratio compared with a conventional interferometer under the same operating condition, which
124    The second is a high-resolution Michelson interferometer used as a phase-sensitive reflection-type
125 hown experimentally to be a robust spin wave interferometer using the forward volume mode, with a lar
126  of magnitude DL attained with label-free PS interferometers using conventional effective optical thi
127 ce, it is essential to demonstrate spin wave interferometers using spatially isotropic spin waves wit
128                                 Conventional interferometers usually utilize beam splitters for wave
129 icroscopy and image analysis, a Mach-Zehnder interferometer was constructed in which one of two inter
130                  In addition, a packaged MCF interferometer was transferred into field trials to vali
131 use nonlinear processes are involved in this interferometer, we can couple a variety of different wav
132 sing a custom-built heterodyne low-coherence interferometer, we demonstrate in living mouse cochleae
133  the cochlear partition using a custom-built interferometer, we demonstrate that electrical stimulati
134      Depending on the operating point of the interferometer, we demonstrated binary and ternary logic
135 e spatial-light-modulator-based polarization-interferometer, we have constructed a 'Hilbert-space ana
136 nt technique based on a scanning Fabry-Perot interferometer, we observe long-living narrowband compon
137                                   Using this interferometer, we obtain interference fringes in a Mach
138 ers into subwavelength cavities of plasmonic interferometers, we demonstrate coherent generation of s
139                                      Our MCF interferometers were used for sensing strain.
140 s in ballistic trilayer graphene Fabry-Perot interferometers, which result from phase coherent transp
141                                  Matter-wave interferometers, which split and recombine wave packets
142       This allows us to fabricate simple MCF interferometers whose interrogation is carried out with
143                           Here we propose an interferometer with a levitated, optically cooled and th
144 contrast CT setup consisting of a Talbot-Lau interferometer with a rotating anode x-ray tube and a si
145                                 Employing an interferometer with a Sagnac-like ring design, we succes
146                              The first is an interferometer with recoiling mirrors.
147 were performed by using a Talbot-Lau grating interferometer with the beam direction in anterior-poste
148 tronomy Observatory's Very Large Array radio interferometer with the Very Long Baseline Array antenna
149 tem consists of a cascade of 15 Mach-Zehnder interferometers with 30 thermo-optic phase shifters inte
150 erfect absorber," functions as an absorptive interferometer, with potential practical applications in

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