An emission spectrum is run 选择语言:从中文简体中文翻译英语日语韩语俄语德语法语阿拉伯文西班牙语葡萄牙语意大利语荷兰语瑞典语希腊语捷克语丹麦语匈牙利语希伯来语波斯语挪威语乌尔都语罗马尼亚语土耳其语波兰语到中文简体中文翻译英语日语韩语俄语德语法语阿拉伯文西班牙语葡萄牙语意大利语荷兰语瑞典语希腊语捷克语丹麦语...
4.6.2 Optical emission and absorption spectra Emission (fluorescence or phosphorescence) spectrum is essential for the color of OLED display device, in addition to providing information on dynamics of ultrafast phenomena and/or the structure parameters. We firstly compared the calculated optical spectra ...
theD-lines of the emission spectrum ofsodiumare found as absorption lines in the same position (i.e. of the same wavelengths) when “white” light is passed throughsodium vapour. Those substances in the outer atmosphere of the sun which absorb radiation from the inner regions of the sun and...
atoward the Zn2þ center. Selective binding of anion to the Zn2þ[translate] aemission changes of 1 (L2 3 Zn2þ) upon the addition of F,[translate] a2-, Pi, PPi, ATP,[translate] aemission spectrum of 1 is characterized by an intense emission[translate]...
We used the OLED display of an Android phone (Google Pixel 2016) as the incoherent light source for encoding input vectors in our experimental setup. Only green pixels (with an emission spectrum centered around 525 nm) were used in the experiments; the OLED display contains an array of ~...
We present an empirical template spectrum suitable for fitting/subtracting and studying the FeII and FeIII line emission in the restframe UV spectra of active galatic nuclei (AGNs), the first empirical UV iron template to cover the full 1250 - 3090 A range. Iron emi...
An ultra-deep IRS spectrum to search for Halpha emission from the galaxies which reionized the Universe 来自 ResearchGate 喜欢 0 阅读量: 18 作者:M Lacy,A Bunker,JP Kneib,H Teplitz 摘要: The ionizing radiation produced by the known population of z~6-7 galaxies falls short of that required...
To observe a well-defined temporal order, that is, a time crystal with a long-range temporal correlation or a long coherence time, it is critical to set a proper optical driving field. Noting that the spectrum of \({P}_{{{\mbox{in}}}=9.5\) mW in Fig. 3a has the narrowest lin...
The emission spectrum is obtained by exciting the luminescence with a particular wavelength. The intensity of the emission is then plotted as a function of wavelength. The excitation spectrum measures the emission at a particular wavelength (usually the wavelength of maximum emission). One may excite...
The spectral line-width of spontaneous emission can be calculated to be 1.8kT(see, e.g.,Schubert, 2006). The theoreticalemission spectrumis shown inFigure 2. The line-width of 1.8kTis caused by thethermal energyof carriers and is therefore referred to as the ‘thermal broadening.’ It indic...