spectral line oor Koreaans
spectral line
en
(physics) a dark or bright line in an otherwise continuous spectrum caused by the absorption or emission of light, at a single wavelength, by the movement of electrons between energy levels of an atom or molecule
Vertalings in die woordeboek Engels - Koreaans
스펙트럼선
en
optical phenomenon
Geskatte vertalings
Vertoon algoritmies gegenereerde vertalings
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These spectral lines, which can only be seen in very low density gases, are called forbidden lines.
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This was done by making sensitive measurements of the Doppler shift of the spectral lines of Gliese 876.
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These energy transitions often lead to closely spaced groups of many different spectral lines, known as spectral bands.
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Significantly, apart from a few nearby galaxies, all known galaxies have spectral lines that are redshifted.
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Prototype for the characteristic LBV spectral lines.
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Secondly, the red shift of the spectral lines would be so great that the spectrum would be shifted out of existence.
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It was built by NASA's Jet Propulsion Laboratory, and incorporated a set of 48 filters isolating spectral lines of particular astrophysical interest.
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Astronomers still differ over whether to classify at least one of the stars as a supergiant, based on subtle differences in the spectral lines.
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The first explains the splitting and polarisation of the spectral lines in a magnetic field.
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Radial velocity is measured by the doppler shift of the star's spectral lines, and is given in units of km/s .
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Spectral lines are shifted towards the red end of the spectrum, from which its distance is determined using the standard LCDM cosmology.
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His important treatise Atomic structure and spectral lines which ran to six editions, reflects the development of theoretical spectroscopy between 1916 and 1946.
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For those stars the terms "dwarf" and "giant" refer to differences in spectral lines which indicate if a star is on the main sequence or off it.
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Edward Pickering discovered the first spectroscopic binary in 1899 when he observed the periodic splitting of the spectral lines of the star Mizar in a 104-day period.
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At first the theory met resistance but, due to the successful work of Niels Bohr in 1913 calculating positions of spectral lines using the theory, it became generally accepted.
본 발명은, 힘의 모멘트의 원리 및 빗면마찰과 탄성의 원리 등을 이용한 갈고리바늘과 루프로 구성되는 일방향성찍찍이에 관한 것이다. 종래 벨크로를 비롯한 자동길이조절 버클, 회전 갈고리형 버클, 톱니형 미세 길이조절 버클 등의 체결기구는, 결속력이 강력하면서도 동시에 소형화하는 데에는 한계점이 있으며, 여러 기술분야에 걸쳐 만족할만한 체결기구는 드문 실정이다.ParaCrawl Corpus ParaCrawl Corpus
He succeeded in arranging the spectral lines of helium in two spectral series and, until 1897, this was thought to be evidence that hydrogen was a mixture of two elements.
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His explanation covered the absorption and excitation of spectral lines and the correspondence principle which he had set out in three papers On the quantum theory of spectra between 1918 and 1922.
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Within a year Runge had moved away from pure mathematics to study the wavelengths of the spectral lines of elements other than hydrogen (J J Balmer had constructed a formula for the spectral lines of helium.)
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However, despite being a mathematics teacher and lecturer all his life, Balmer is best remembered for his work on spectral series and his formula, given in 1885, for the wavelengths of the spectral lines of the hydrogen atom.
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Rather than a strong continuum with absorption lines superimposed, the Orion Nebula and other similar objects showed only a small number of emission lines .[7] In planetary nebulae , the brightest of these spectral lines was at a wavelength of 500.7 nanometres , which did not correspond with a line of any known chemical element .
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Pauli eagerly accepted the invitation and spent the year 1922-23 at Bohr's Institute : Following Bohr's invitation, I went to Copenhagen in the autumn of 1922, where I made a serious effort to explain the so-called 'anomalous Zeeman effect', ... a type of splitting of the spectral lines in a magnetic field which is different from the normal triplet.
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Ultraviolet astronomy is best suited to the study of thermal radiation and spectral emission lines from hot blue stars (OB stars ) that are very bright in this wave band.
이에 의해, 최적의 테마가 사용자 맞춤형으로 제공되어, 사용자가 시각적인 즐거움과 신선함을 느낄 수 있도록 하여 준다.ParaCrawl Corpus ParaCrawl Corpus
Physicists showed in the 1920s that in gas at extremely low density , electrons can populate excited metastable energy levels in atoms and ions , which at higher densities are rapidly de-excited by collisions.[10] Electron transitions from these levels in doubly ionized oxygen give rise to the 500.7 nm line.[11] These spectral lines , which can only be seen in very low density gases, are called forbidden lines .
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Their three-dimensional display in a 3D spectrum allows for a correct evaluation of the absorption lines and their spectral background.
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Following this line he published papers which introduced sheaves, and the spectral sequence of a continuous map.
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29 sinne gevind in 10 ms. Hulle kom uit baie bronne en word nie nagegaan nie.