山东地区典型金属罐喷涂企业VOCs排放特征研究     

曹双  高素莲  闫学军  刘光辉  王琛 《南京气象学院学报》2020,12(6):749-757

了解涂装行业挥发性有机物（VOCs）的排放特征是制定山东地区臭氧（O₃）和PM_2.5防控策略的重要环节.本研究在山东地区测定了两家典型食品金属包装企业喷涂过程中VOCs的排放组成,企业产品以饮料罐和罐头为主.结果表明：两家企业排放的总VOCs质量浓度水平相当,质量浓度变化范围在50~1 500 μg/m³;但两家企业喷涂过程中VOCs的排放组成具有一定的差异,以生产铝罐和马口铁罐为主的企业中的含氧挥发性有机物（OVOCs）含量最多,占比89.71%（质量分数,下同）;而生产铝罐的企业芳香烃（56.15%）是首要的排放种类,其次是OVOCs （32.32%）.通过分析两家企业内外喷涂工艺的VOCs源成分谱,发现同一企业不同工艺之间有一定差异,多种罐生产企业的内、外喷涂中乙醇占比最高,分别为94.28%、84.46%;单铝罐生产企业的内喷涂2-丁酮（24.33%）是重要组分,外喷涂中甲苯（36.40%）含量较高.  相似文献   

Accurate laboratory ultraviolet wavelengths for quasar absorption-line constraints on varying fundamental constants     

M. Aldenius  S. Johansson  M. T. Murphy 《Monthly notices of the Royal Astronomical Society》2006,370(1):444-452

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Hyperfine structure of the ground state in singly ionized manganese     

R. J. Blackwell-Whitehead  A. Toner  A. Hibbert  J. Webb  S. Ivarsson 《Monthly notices of the Royal Astronomical Society》2005,364(2):705-711

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The iron Kα lines as a tool for magnetic field estimations in non-flat accretion flows     

A.F. Zakharov  Z. Ma  Y. Bao 《New Astronomy》2004,9(8):663-677

Observations of AGNs and microquasars by ASCA, RXTE, Chandra and XMM-Newton indicate the existence of broad X-ray emission lines of ionized heavy elements in their spectra. Such spectral lines were discovered also in X-ray spectra of neutron stars and X-ray afterglows of GRBs. Recently, Zakharov et al. [MNRAS 342 (2003) 1325] described a procedure to estimate an upper limit of the magnetic fields in regions from which X-ray photons are emitted. The authors simulated typical profiles of the iron Kα line in the presence of magnetic field and compared them with observational data in the framework of the widely accepted accretion disk model. Here we further consider typical Zeeman splitting in the framework of a model of non-flat accretion flows, which is a generalization of previous consideration into non-equatorial plane motion of particles emitting X-ray photons. Using perspective facilities of space borne instruments (e.g., Constellation-X mission) a better resolution of the blue peak structure of iron Kα line will allow to evaluate the magnetic fields with higher accuracy.  相似文献   

活动星系核（AGN）的宽线区（BLR）（Ⅱ）     

薛随建  程福臻 《天文学进展》1995,13(1):84-90

ＡＧＮ天体的主要特征之一，就是它们的光谱中有宽而强的发射线，因此，这些宽发射线的产生区域ＢＬＲ为人们提供了一个了解ＡＧＮ天体物理本质的独特而重要的场。在文中围绕讨论了ＢＬＲ基本物理特征，评述近年来有关的理论和观测研究进展及其现状在文（Ⅱ）中主要涉及ＢＬＲ的几何结构和尺度及其运动学研究的进展和现状。  相似文献   

Getting SMARTS on Novae: Highlights of the Early Evolution of Nova V475 Sct     

Guy S. Stringfellow  Frederich M. Walter 《Astrophysics and Space Science》2006,304(1-4):401-403

There is a disconcerting global trend of retiring telescopes of modest aperture, supplanting them instead with fewer expensive telescopes of quite large aperture. As a consequence, the available time and feasibility of following transient objects in astrophysics is diminishing. We show the utility of having a suite of small to moderate aperture telescopes capable of conducting imaging and spectroscopic observations in a service queue mode. The example we provide is the high-cadence early observations of the classical nova V475 Scuti (2003) carried out with the SMARTS suite of telescopes located at CTIO.  相似文献   

Relativistic emission lines from accretion discs around black holes     

Andrej &#;ade&#;  Massimo Calvani 《Monthly notices of the Royal Astronomical Society》2005,363(1):177-182

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Limits on the 2.2-μm contrast ratio of the close-orbiting planet HD 189733b     

J. R. Barnes  Travis S. Barman  L. Prato  D. Segransan  H. R. A. Jones  C. J. Leigh  A. Collier Cameron  D. J. Pinfield 《Monthly notices of the Royal Astronomical Society》2007,382(1):473-480

We obtained 238 spectra of the close-orbiting extrasolar giant planet HD 189733b with resolution   R ∼ 15 000  during one night of observations with the Near-Infrared High-Resolution Spectrograph (NIRSPEC), at the Keck II Telescope. We have searched for planetary absorption signatures in the  2.0–2.4 μm  region where H₂O and CO are expected to be the dominant atmospheric opacities. We employ a phase-dependent orbital model and tomographic techniques to search for the planetary absorption signatures in the combined stellar and planetary spectra. Because potential absorption signatures are hidden in the noise of each single exposure, we use a model list of lines to apply a spectral deconvolution. The resulting mean profile possesses a signal-to-noise ratio (S/N) that is 20 times greater than that found in individual lines. Our spectral time series thus yields spectral signatures with a mean S/N = 2720. We are unable to detect a planetary signature at a contrast ratio of  log₁₀( F _p/ F _*) =−3.40  , with 63.8 per cent confidence. Our findings are not consistent with model predictions which nevertheless give a good fit to mid-infrared observations of HD 189733b. The 1σ result is a factor of 1.7 times less than the predicted 2.185-μm planet/star flux ratio of  log₁₀( F _p/ F _*) ∼−3.16  .  相似文献   

Polarization of the broad Hα wing in symbiotic stars     

Jerry Jaiyul Yoo  Jih-Yong Bak  Hee-Won Lee 《Monthly notices of the Royal Astronomical Society》2002,336(2):467-476

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Temporal fluctuations in the differential rotation of cool active stars     

J.-F. Donati  A. Collier Cameron  P. Petit 《Monthly notices of the Royal Astronomical Society》2003,345(4):1187-1199

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