「spectral」の共起表現一覧(1語右で並び替え)

spectral

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  • Photochromic pigments change their "colour" ( spectral absorbance properties) upon light absorption.
  • spectral absorption maxima (in solution)
  • The Fraunhofer lines are typical spectral absorption lines.
  • Spectral acceleration (SA) is a unit measured in g (th
  • d on a 2% probability of exceeding 0.2 second spectral acceleration at 5 Hz in 50 years
  • Spectral acceleration, with a value related to the nat
  • e seismic hazard maps are also produced using spectral acceleration.
  • ate of the center of the peak, thus improving spectral accuracy.
  • For example in spectral analysis the expected peak shape is often kno
  • and synthesis techniques, including real time spectral analysis and additive resynthesis, audio morp
  • rospectrophotometers used for non-destructive spectral analysis and imaging of microscopic sampling
  • observatory is particularly well situated for spectral analysis in astronomy, which requires a clear
  • analysis, then the method is called Gradient spectral analysis (GSA), usually applied to short time
  • al operations such as electronic filters, for spectral analysis and for synchronized display of data
  • However, in 2005, an extensive mass spectral analysis showed that the actual structure is
  • Spectral analysis of the least volatile fraction revea
  • the measurements of atmospheric electricity, spectral analysis of rare-earth elements, wave guide t
  • For the spectral analysis technique, see Least-squares spectra
  • Spectral analysis has shown traces of ice.
  • Maximum entropy spectral analysis (MaxEnt spectral analysis) is a meth
  • Spectral analysis and its applications (with D. G. Wat
  • Detailed X-ray spectral analysis has been performed on 123 X-ray sour
  • The multitaper spectral analysis is a powerful nonparametric method t
  • Spectral analysis of Egeria shows it to be unusually h
  • Advanced systems also perform spectral analysis, ischemic burden evaluation, graph o
  • ach height in registers or channels for later spectral analysis.
  • Model 1 suffers from the fact that the spectral and temporal characteristics strongly resembl
  • ured work from artists such as Total Eclipse, Spectral, and Voodoo People.
  • 18 Scorpii is a main sequence star of spectral and luminosity type G2 Va.
  • , comprising Alnitak Aa (a blue supergiant of spectral and luminosity type O9.7 Ibe, with an absolut
  • serial, atonal, microtonal, polymodal, spectral and others, however his style has emerged int
  • Spectral and harmonic response
  • d (sensor calibration, orbital drift, limited spectral and directional sampling, etc.).
  • Each spectral appearance precedes a tragic event on the rai
  • nds her ground against General Hadias and the Spectral army in Australia, and the mighty Great Mazin
  • ital alongside other similarly dressed men, a spectral army clutching briefcases and silently marchi
  • Casting Eternal Fires Volume 1 ( Spectral Arts Productions, 2002)
  • Developed by Spectral Associates in 1981, the game lulls players in
  • Spectral attenuation of fiber optics
  • Bathochromic shift is a change of spectral band position in the absorption, reflectance,
  • HDC (Hybrid Digital Coding) with SBR ( spectral band replication) is a proprietary lossy audi
  • The instruments capture data in 36 spectral bands ranging in wavelength from 0.4 µm to 14
  • m resolution in two visible and two infra-red spectral bands over two 100km swathes; "Visible and Th
  • HyMap data has 126 spectral bands spanning the wavelengh interval 0.45-2.
  • ging Self Scanner (LISS-4) operating in three spectral bands in the visible and Near Infrared Region
  • ring the 2009 and 2010 seasons in the K and L spectral bands.
  • lasers requires the exponential growth of the spectral bandwidth of gain and/or length of partial la
  • o be confused with the namesake SBasic (S for Spectral Basic) Programming Language for the commercia
  • He is commander of the Spectral Battle Beasts, one of the Seven Armies of the
  • urces for infrared spectroscopy because their spectral behaviour corresponds approximately to that o
  • gnus' demonic knights and now an intimidating spectral blue demonic aura, the demon Yamato, hovers a
  • designed to deliver photons with high average spectral brightness in the 2 keV to 10 keV energy rang
  • trum to compare with other stars in a similar spectral category.
  • f the progenitor, accounting for the observed spectral changes.
  • Its spectral characteristics are unknown.
  • The spectral characteristics of the supernova changed over
  • s apparent magnitude +3.02 and belongs to the spectral class K2 III.
  • Lambda Ophiuchi belongs to spectral class A1V+A and has apparent magnitude +3.82.
  • J Centauri is a spectral class B3V main sequence star with a mean appa
  • Classical Cepheids are yellow supergiants of spectral class F6 - K2 and their radii change by (~25%
  • Misam belongs to the spectral class K0 and has apparent magnitude +3.8.
  • The companion is a spectral class M0.5V red dwarf star with absolute magn
  • d has an apparent magnitude of 2.72 and is of spectral class K3, giving it a decidedly yellowish ora
  • Ardelean is a binary star, consisting of a spectral class A2 giant with an apparent magnitude of
  • It has apparent magnitude +2.7 and belongs to spectral class B2.
  • as apparent magnitude +3.1 and belongs to the spectral class A0.
  • ive member has approximately 20 solar masses ( spectral class O8 V).
  • Alchiba belongs to the spectral class F0 and has apparent magnitude +4.00.
  • It is of spectral class A3, and is approximately 99 light years
  • It is the closest spectral class L brown dwarf to the Earth.
  • ary star is classified as a blue-white dwarf ( spectral class B2.5 V).
  • Alpha Monocerotis belongs to the spectral class G9 and is of apparent magnitude 3.93.
  • Miram belongs to spectral class K3 and has an apparent magnitude of +3.
  • r is classified as a yellow-white supergiant ( spectral class F8 Iab).
  • apparent magnitude of +3.5 and belongs to the spectral class F0.
  • Gliese 435 (HD 101581, HIP 56998) is a K5 V e spectral class stellar object located 40.9 light years
  • e star is classified as a yellow-white giant ( spectral class F2 III).
  • It is an orange dwarf ( spectral class K2V), somewhat dimmer and cooler than o
  • It is a red giant of the spectral class M3, with a surface temperature of 3,650
  • It belongs to the spectral class T8V; its surface temperature is 600-750
  • pparent magnitude of +2.88 and belongs to the spectral class F2II.
  • f apparent magnitude +3.25 and belongs to the spectral class M3-III.
  • It is a wide binary of spectral class B stars, each of magnitude 4.0 and 5.1.
  • Its distance is about 108 light years and spectral class is K1III.
  • Omega Herculis belongs to spectral class B9pCr and has apparent magnitude +4.58.
  • Iota Leonis is of the spectral class F4IV and apparent magnitude +3.94.
  • Ancha belongs to the spectral class G8 and has an magnitude of +4.17.
  • considered normal for a main sequence star of spectral class M. The proportion of elements with atom
  • The binary's composite spectral class is F9V and its combined apparent magnit
  • Its spectral class is intermediate between the C-type and
  • ittae B is a probably a substellar L dwarf of spectral class L6±1.5 orbiting primary 15 Sagittae A.
  • Iota Ceti belongs to spectral class K1.5III and has apparent magnitude +3.5
  • Delta Scuti variables typically range from spectral class A2 to F8, and a stellar luminosity clas
  • editors to change the category along with the spectral class in the table.
  • y star system BD+31°643, which has a combined spectral class of B5.
  • Gamma Ceti belongs to spectral class A2 and has apparent magnitude +2.7.
  • he main sequence star is a red dwarf with the spectral class M3.5V.
  • It belongs to the spectral class T2.5 and its position shifts due to its
  • Eta Lyrae belongs to spectral class B2.5IV and has apparent magnitude of +4
  • Eta Pegasi is of spectral class G2II-III and has apparent magnitude +3.
  • mers categorize it as a main-sequence star of spectral class K2, which means the energy being genera
  • 41 Arietis belongs to the spectral class B8Vn, and has a stellar magnitude of +3
  • Persei has an apparent magnitude of +4.7 and spectral class A2V.
  • Albali belongs to the spectral class A0 and has an apparent magnitude of +3.
  • ht giant star of apparent magnitude +4.37 and spectral class G1 II about 475 light years from Earth.
  • e enabled an observer to deduce the color and spectral class of a star very easily.
  • 46 LMi has spectral class K0+III-IV and is of magnitude 3.83.
  • Mu Leonis is of spectral class K3 and apparent magnitude +4.1.
  • Sigma Puppis belongs to spectral class K5 and has apparent magnitude +3.3.
  • maller and less luminous than our Sun, with a spectral class of K3V, which makes it an orange-red hu
  • s apparent magnitude +4.67 and belongs to the spectral class B3IV.
  • It has spectral class M2 and is of apparent magnitude 3.5.
  • Alpha Equulei collectively belongs to spectral class G0III and has apparent magnitude +3.92
  • Alpha Hydri belongs to spectral class F0V and has apparent magnitude +2.9.
  • o of 0.19 is too high, and it is of the wrong spectral class to be part of the dark carbonaceous Hyg
  • Some Sun-like stars of spectral class F8 to G8 have been found to undergo eno
  • Xi Geminorum belongs to spectral class F6 and has apparent magnitude +3.4.
  • It belongs to the spectral class T7, its surface temperature is 800-1300
  • Beta Piscium belongs to the spectral class B6Ve and is of magnitude +4.53m.
  • Each is of the spectral class F7V and has a visual magnitude of 5.8m.
  • Earth, consisting of a magnitude 5.44 star of spectral class M2 and a 6.6 magnitude star of spectral
  • It is an orange dwarf star of spectral class K5, orbiting the yellow giant at about
  • 8 Aquarii is a blue-white sub-giant of the spectral class A4IV in the constellation Aquarius with
  • Alpha Crateris belongs to the spectral class K1, has apparent magnitude 4.07, and is
  • (absolute magnitude −0.7) and belongs to the spectral class A0.
  • of +4.042 and is classified as a blue giant ( spectral class O7.5III).
  • Gamma Librae belongs to the spectral class K0III, and is of the fourth-magnitude,
  • The two stars of Subra are of spectral class F9III (a giant star) for the primary an
  • d-magnitude) and is a blue giant belonging to spectral class B8III.
  • light years from the Earth and belongs to the spectral class B9.5V.
  • R Hydrae's spectral class is M7IIIe.
  • It has a spectral class of K1e and is located 39.9 light-years
  • a yellow star of apparent magnitude 3.88 and spectral class F2 III about 61 light years from Earth.
  • visible to the naked eye, and belongs to the spectral class B5III.
  • rateris is a white sub-giant belonging to the spectral class A2, has apparent magnitude 4.48, and is
  • The spectral class of the star is Am.
  • Persei has an apparent magnitude of +4.63 and spectral class K1 III lying about 305 light years from
  • τ Pegasi belongs to the spectral class A5Vp.
  • It has spectral class A0 and is of magnitude 3.3.
  • The brightest companion, η Sagittarii B, is spectral class F dwarf star, with an apparent magnitud
  • a yellow star of apparent magnitude 4.08 and spectral class F6 III about 70 light years from Earth.
  • Gliese 349 is a star with a K3Ve spectral class and a radial velocity of +27.6 km/s, lo
  • The spectrum matches a giant star of spectral class G7Ib-II.
  • ghtness of +4.13 magnitude and belongs to the spectral class F5IV; a subgiant star.
  • t was on the main sequence, it probably was a spectral class B star (in the range B4-B9).
  • tar with an apparent magnitude of +3.17 and a spectral class of B9.
  • Theta Cygni is a white main sequence star, spectral class F3 V, forming a wide binary system with
  • The star is classified as a blue-white dwarf ( spectral class B4 Vn).
  • It is a G-type giant star, with spectral class G2 and an apparent visual magnitude of
  • aconis has apparent magnitude +3.75 and is of spectral class K2-III.
  • 53 Eridani belongs to the spectral class K2IIIb and has apparent magnitude +3.87
  • The star is classified as an orange giant ( spectral class K1 III).
  • lorum is a supergiant or bright giant star of spectral class K5.
  • It contains many spectral class O- and B-type stars, and may represent
  • Beta Aquilae has magnitude 3.71 and is of spectral class G8IV.
  • This system consists of a spectral class B3 star being orbited by a less massive
  • Gliese 208 is an orange dwarf star (K7 spectral class) with an apparent magnitude of 8.9.
  • HIP 105766 is a potential Sun-like star (G5 spectral class) with an apparent magnitude of 7.3.
  • liese 710 is a variable orange dwarf star (K7 spectral class) in the constellation Serpens Cauda, wi
  • not expected to originate from a star of this spectral class.
  • There is some uncertainty as to its spectral class.
  • ally related to the group, being of the wrong spectral class.Yet, NASA continues to categorize it as
  • The A6 part is the spectral class: the A indicates this is a white star s
  • oped the system of classifying stars into the spectral classes O, B, A, F, G, K, M.
  • evolution, along with main sequence stars of spectral classes A, F, G, K, and M.
  • The movement of stars of spectral classes B and A around the apex (left) and an
  • atoms and light related to the history of the spectral classes.
  • If the spectral classification is performed including the met
  • e main star is of apparent magnitude +1.6 and spectral classification M4 III.
  • It has a spectral classification of K2, giving it an orange-red
  • Spectral classification places it between a dwarf and
  • apparent magnitude of +2.1 and belongs to the spectral classification B3.
  • The MK system remains the standard stellar spectral classification system used by astronomers tod
  • apparent magnitude of +1.5 and belongs to the spectral classification B2.
  • White dwarfs whose primary spectral classification is DA have hydrogen-dominated
  • ellman (1911-2007) to develop the MKK stellar spectral classification system between 1939 and 1943.
  • It has a spectral classification of K0 V and has about 86% of t
  • The Morgan-Keenan spectral classification
  • Based on its spectral classification of G0 V, it is similar in mass
  • n apparent magnitude of +2.08, belongs to the spectral classification A5, and is about 47 light year
  • 2 stars are on the smaller end of the Harvard spectral classification list, solely being larger than
  • The composite spectral classification of the AB pair is G0V, which d
  • rked on problems of stellar statistics and on spectral classification of stars, publishing the Bonn
  • that carbon and metals are not present, which spectral classification is seen depends on the effecti
  • Its +6.4 magnitude white companion star ( spectral classification A3) lies about 2 arcminutes aw
  • Its spectral classification has been measured as A0 and al
  • e in brightness is accompanied by a change in spectral classification, from G1 to F4.
  • Based on its spectral classification, it is slightly less massive a
  • GJ 440 has a DQ spectral classification, indicating that it is a rare
  • nent reddish-orange, well in keeping with its spectral classification.
  • Measurement of the spectral coherence of light requires a nonlinear optic
  • recious opal, where brilliant regions of pure spectral color result from close-packed domains of col
  • A spectral color is a color that is evoked by a single w
  • Every wavelength of light is perceived as a spectral color, in a continuous spectrum; the colors o
  • While such a massive spectral compilation itself was something of a tour de
  • spectral) complex impedance, equivalent to the amount
  • xcipients, each of which will produce a Raman spectral component with a relative intensity proportio
  • requires a method to separate the individual spectral components and correlate their intensity cont
  • us signal and analyzing the resultant output, Spectral Contamination testing provides a measure of a
  • and different sources of noise have different spectral content.
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