「Emission」の共起表現一覧(1語右で並び替え)
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| While induced | emission adds only power to a radiation field, stimula |
| There is no performance or | emission advantage when the CN is raised past approxim |
| Nord Pool started trading and clearing of EU | emission allowances, becoming the first exchange to ex |
| Hα | emission also has spiral structure which is surprising |
| Thus, EE is an electron | emission analogue of such optical phenomena as phospho |
| lectronics that involved cathodes, electronic | emission, and gaseous conduction. |
| cket Radar utilizes the same microwave signal | emission and detection methods found in the Doppler sp |
| The Advanced Spaceborne Thermal | Emission and Reflection Radiometer (ASTER), an Earth o |
| al component of the velocity of the source at | emission and the observer at observation, as determine |
| ngle with a height equal to that of continuum | emission, and finding the width such that the area of |
| the chemical substrate between absorption and | emission and is extremely fast, of the order of 10 nan |
| s is one of many forms of luminescence (light | emission) and is distinguished by photoexcitation (exc |
| cal peculiarities, nuclear radio and infrared | emission, and starburst or active galactic nuclei (AGN |
| ASTER (Advanced Spaceborne Thermal | Emission and Reflection Radiometer) is a Japanese sens |
| The tops represent light | emission and nucleotide binding. |
| ASTER (Advanced Spaceborne Thermal | Emission and Reflection Radiometer) |
| stainable methods of transport, favouring low | emission and public transport over high emission, priv |
| NGC 6072 also shows H2 (Hydrogen) | emission and intense CO (Carbon Monoxide) emission whi |
| olecule, it cannot lose this energy by photon | emission, and its excited vibrational levels are there |
| nonlinearities, band-gap effects, spontaneous | emission, and other such research endeavors. |
| ed of these is 8C which decays through proton | emission and alpha decay and has a half-life of 1.9873 |
| High current densities produce continuum | emission and tend to favor shorter wavelengths. |
| ntradictions when applied to the phenomena of | emission and transformation of light. |
| sis, nulling the relationship between methane | emission and NEP because methane production becomes de |
| This causes a peak in the total radiation | emission and can be well detected. |
| around 570 nanometres, that matched emerald's | emission and absorption characteristics, this filter w |
| e influence on density on the position of the | emission and absorption lines in a gas spectrum" and w |
| f Mathematical Models of Electromagnetic Wave | Emission and Propagation in Photonic Band-Gap Material |
| n through a medium is affected by absorption, | emission and scattering processes. |
| ist, known for his research on field electron | emission and field ionization, and his role as an advi |
| He is the author of Field | Emission and Field Ionization (American Vacuum Society |
| d two-level atom the detailed balance for the | emission and absorption which preserves the Max Planck |
| n the excitation potentials of metals and the | emission and absorption of soft X-rays by solids (1932 |
| coefficients) for the absorption, spontaneous | emission, and stimulated emission of electromagnetic r |
| COROT-7b in and out of transit, searching for | emission and absorption lines originating in the exosp |
| adius of which is a measure for the Cherenkov | emission angle. |
| On the contrary, the | emission area in the case of tip injection depends on |
| The | emission area for substrate injection is homogeneous a |
| They used amplified spontaneous | emission as a probe to study self healing properties. |
| ill also provide maps of Galactic synchrotron | emission at lowest frequencies. |
| The gamma | emission at 1809 keV was the first observed gamma emis |
| The star system does not show any excess | emission at 70 μm, indicating it does not have a cold |
| ngth between the points on either side of the | emission at an average intensity between the K1 minimu |
| dered as an important contaminating source of | emission at very long infrared wavelengths (λ > 300 µm |
| if the Apollo astronaut sightings of diffuse | emission at 10s of km above the surface were Na glow o |
| the physical processes associated with energy | emission at these wavelengths, scientists can calculat |
| ons at centimeter wavelengths with DIRBE dust | emission at 140 μm, while Leitch et al had correlated |
| Excitation with light at ~470 nm results in | emission at ~570 nm. |
| the small observed power of the doublet Mg II | emission at 2800 angstrom. |
| current and the realization of the continuous | emission at the room temperature |
| cally optimised pantographs for reduced noise | emission atop cars 4 and 9. |
| himself attempted to resolve the hydrogen Hα | emission band in the spectrum of a hydrogen atom into |
| C2 | emission bands were observed in the comet Skorichenko- |
| time the details of the fine-structure of the | emission bands and the absorption edges. |
| The position of the absorption and | emission bands remain almost unchanged in solvents of |
| uous Descent Approaches (CDAs) have noise and | emission benefits in low traffic environments based up |
| It is a zero CO2 | emission building showing a new model of green archite |
| regular routes run with modern low floor, low | emission buses. |
| appears as a very bright North-South ridge of | emission, but it extends far to the East and can be de |
| r the expected background of diffuse Galactic | emission, by the SAS-2 satellite (Fictel et al. 1975) |
| e, did not reduce Jovian decametric radiation | emission by contributing significant dust to the Jovia |
| Emission can also be induced by other sources of energ | |
| e, longer bulb life from dimming, and reduced | emission carbon footprints. |
| f the car tax law for the introduction of low | emission cars and the detergent Act of March 5, 1987. |
| protocol is implemented through the National | Emission Ceilings (NEC) directive. |
| und the P-side contacts reach the part of the | emission characteristics with lower brightness/current |
| e chosen to match the spectral excitation and | emission characteristics of the fluorophore used to la |
| In FRI sources the major part of the radio | emission comes from closer to the centre of the source |
| pplications on interactive binaries resolving | emission components such as the inner face of the comp |
| Gaseous | emission concentration, composition and flux as well a |
| Emission considerations require the evaluation of many | |
| Emission contribution from structures with large-scale | |
| removal of the precisely determined zodiacal | emission contribution (which was based on the measured |
| ineration plants to achieve high standards of | emission control more effectively. |
| The decrease is due to strict | emission controls and also to the control of concentra |
| etermination that increased the stringency of | emission controls in the Baton Rouge area, and obtaine |
| Thermotunnel cooling is similar to thermionic | emission cooling in that fast moving electrons carry h |
| the width of the | emission core of the K line ( W0 ) can be measured in |
| Zoom on the | emission core. |
| roperties determine the magnitude of electron | emission current and electric potential at the electro |
| in a microscope is very similar to Stimulated | Emission Depletion Microscopy, however it can operate |
| J0437-4715 is the first MSP to have its X-ray | emission detected and studied in detail. |
| contains many dark nebulae in addition to the | emission diffuse nebulae. |
| The | emission direction is random. |
| This effect of prompt neutron | emission does not permit to obtain primary primary mas |
| te Houtermans The Relative Secondary Electron | Emission Due to He, Ne, and A Ions Bombarding a Hot Ni |
| Here, quantum yield is essentially the | emission efficiency of a given fluorophore in this cas |
| From 1978 to 1980, to reduce pollutant | emission, electrical filters were added to the plant. |
| In 1964 Crewe developed the first field | emission electron gun, a new type of electron source t |
| f sight of the observer, one can detect radio | emission emitted near the star's magnetic poles. |
| ntensity on either side of the absorption (or | emission) feature, while Fλ represents the intensity a |
| f a star made by recreating the absorption or | emission features seen in the spectrum. |
| ater scientific study noted that the official | emission figures were consistent with available dosime |
| , using the relatively low official radiation | emission figures, "The average radiation dose to peopl |
| Based on these low | emission figures, early scientific publications on the |
| on that refers to a bright complex of optical | emission filaments in the southwest part of the shell, |
| mirror (or dichromatic beamsplitter), and the | emission filter (see figure below). |
| n and narrow-band filters, especially an OIII | emission filter. |
| ed fluorescence through the use of a spectral | emission filter. |
| r deep blocking filters (commonly employed as | emission filters). |
| Due to different time of light | emission for different types of ionizing particles, th |
| me excitation frequency but pass a particular | emission frequency. |
| heating or longwave illumination, not causing | emission from untreated samples. |
| c Microwave Background anisotropy and diffuse | emission from the Galaxy on angular scales from 1 to 5 |
| es where an X-ray spectrum typical of thermal | emission from a cooling neutron was observed. |
| Equally, the | emission from a particular state may be selectively mo |
| resting information on the different modes of | emission from the perspective of the stability of the |
| lation was due to free-free or Bremsstrahlung | emission from ionized gas caused by young hot stars wh |
| "Secondary-electron | emission from complex surfaces". |
| the MWA are to detect neutral atomic Hydrogen | emission from the cosmological Epoch of Reionization, |
| The same satellite discovered X-ray | emission from the same object, and the GMOS Instrument |
| given a protein of known sequence, The X-ray | emission from sulfur can be used as an internal standa |
| announced 45 watt continuous wave single-mode | emission from an optically pumped VECSEL. |
| The X-ray | emission from the source is dominated by thermal emiss |
| region that is characterized by spectral line | emission from weakly ionized atoms. |
| region that is characterized by spectral line | emission from weakly ionized atoms. |
| Compared with other astronomical sources, the | emission from the sun is highly time variable and the |
| Infra-red light | emission from the hot dust torus lags optical light em |
| "Light | Emission from a Moving Source in Connection with the R |
| a-ray bursts), the study of diffuse gamma-ray | emission from the Galactic plane, and a measurement of |
| Observation of X-ray | emission from the collision of Comet Shoemaker-Levy wi |
| in with a thesis entitled Anomalous Microwave | Emission from Bulk Semiconductors. |
| Optical jet | emission from 3C 371 was first detected in ground base |
| The magnitude of methane | emission from a wetland are usually measured using edd |
| ture to be determined, assuming it is thermal | emission from the surface of a neutron star. |
| ounced a detection of strong infrared thermal | emission from the transiting extrasolar planet HD 1897 |
| The observed | emission from a Blazar is greatly enhanced by relativi |
| will be the search for redshifted 21 cm line | emission from the Epoch of Reionization (EoR). |
| pacitance, screen grid current, and secondary | emission from the anode, thus increasing power convers |
| solution is necessary to separate out thermal | emission from the sources' large-scale hot-gas environ |
| X-ray | emission from a limb flare is recorded by Solrad 1 and |
| ghtness and appear to be generated by ongoing | emission from the center of the galaxy. |
| t is used for observations of millimetre wave | emission from molecules in comets, circumstellar envel |
| Problems continued with dioxin | emission from the works incinerator which burned resid |
| Discovery of the iron helium-like | emission from the galactic ridge |
| use the effect (ii) that unexpected microwave | emission from within the solar system is contaminating |
| o the visible are used to excite fluorescence | emission from objects for viewing by eye or with sensi |
| er the next few years, both X-ray and optical | emission from this remnant were also detected, and in |
| , a type of nuclear region with spectral line | emission from weakly ionized gas that could contain ei |
| The gamma ray | emission from this object is of the variety known as a |
| As a result, the neutron | emission from a used fuel element which had included c |
| d with barium, which is likely due to neutron | emission from an undetected white dwarf companion. |
| far right in the figure), shows much greater | emission from the side with varnish than from any of t |
| an unsuccessful attempt to measure the radio | emission from the Sun. |
| fect of Temperature on the Secondary Electron | Emission from Nickel, Phys. |
| Radio | emission from the Andromeda Galaxy was first detected |
| asure (naturally-occurring) microwave thermal | emission from the limb (edge) of Earth's upper atmosph |
| could easily power this X-ray flux, but X-ray | emission from neutron stars is known to be nonthermal, |
| Attempts to detect X-ray | emission from Procyon with nonimaging, soft X-ray sens |
| Purchased all-electric, zero | emission GEM car for use in House of Representatives |
| ion of the empty electronic states, while the | emission gives information about the occupied states. |
| caused the airport to not reach its targeted | emission goals. |
| cientific evidence is indicating that current | emission growth must be stopped and global emissions r |
| the Spitzer Space Telescope, excess infrared | emission has been observed from the star, which can be |
| This | emission has been assigned to the breathing motion of |
| In general, the energy source for LINER | emission has been a subject of debate among astronomer |
| its thermal hard X-rays with a strong Fe XXVI | emission has been found. |
| This | emission has been assigned to the breathing motion in |
| ition may be emitted as a photon (spontaneous | emission), however in practice the 3→2 transition (lab |
| nts based at the facility include the Thermal | Emission Imaging System (THEMIS) on NASA's Mars Odysse |
| n experiment designed to detect the Cherenkov | emission in the radio regime of the electromagnetic sp |
| olecules are frequently less capable of light | emission in terms of brightness and duration when comp |
| scoverer of the element oxygen, because green | emission in the aurora (astronomy), due to atomic oxyg |
| Solar γ-ray | emission in the energy range 0.05 - 300 MeV was observ |
| le, where the presence of both absorption and | emission in the spectral line profile indicate the exi |
| Because of its ‘perylene-type' optical | emission in the visible spectrum, it has also been use |
| The excited molecules then undergo stimulated | emission in the optical resonator region of the laser. |
| ng Radiometer (MSR)" which measures microwave | emission in the 23GHz and 31GHz bands. |
| M.A. in 1905, he began research on thermionic | emission in the Cavendish Laboratory. |
| ition occurs to a higher energy level, or the | emission, in the reverse case, of a photon. |
| These materials show bright | emission in the visible and near infra-red region of t |
| The first term is due to the | emission in every single spectral line. |
| ibed by L.V. Kuhi is: 'The width of the Ca II | emission in normal, nonvariable, G, K, and M stars is |
| as been presented that the ring of soft X-ray | emission includes Cygnus X-6 and Cygnus X-7. |
| Emission indicates that radiative energy is released b | |
| Tour, JM Nanotubes in Microwave Fields: Light | Emission, Intense Heat, Outgassing, and Reconstruction |
| esent can be measured by taking ratios of the | emission intensities of various atomic spectral lines. |
| U.S. EPA Greenhouse Gas | Emission Inventories |
| Greenhouse gas inventories are a type of | emission inventory that are developed for a variety of |
| This | emission is probably from a gaseous disk created by ra |
| emiconductor photodetectors, while stimulated | emission is responsible for laser action in laser diod |
| Band | Emission, is the fraction of the total emission from a |
| The energy | emission is consistent with the model of a merger by c |
| The period between absorption and | emission is typically extremely short, in the order of |
| Such synchrotron | emission is expected from the environment around a sup |
| er gain sections in which seeding spontaneous | emission is amplified with high gain factors of 30 dB |
| iting it, longer and easier to quantify light | emission is often observed. |
| of around 190″ under the assumption that this | emission is uniform around the planetary nebula. |
| nburned fuel is emitted from a combustor, the | emission is caused by fuel "avoiding" the flame zones. |
| s galaxy (as traced by hydrogen spectral line | emission) is also offset from the nucleus. |
| at the centre of the cluster, where the X-ray | emission is brightest. |
| le than the actinides the predominant form of | emission is gamma or beta decay. |
| the faintest star of WR20a, though its X-ray | emission is quite peculiar (see Naze et al. 2008, A&A, |
| is attached or is in proximity to bead, light | emission is stimulated. |
| n if the output power is based on spontaneous | emission it has to be noted that the amplification mec |
| Furthermore, because of the widely tunable QD | emission, it's possible to have near UV-pumped QD-LEDs |
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