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961.
安徽省庐枞盆地高岭土矿的成矿规律、找矿方向及开发应用问题探讨 总被引:1,自引:0,他引:1
庐枞盆地是以中、下侏罗统陆相碎屑岩建造为基底,经燕山运动而发育起来的陆相继承性火山岩盆地,是长江中下游地区重要的矿产地之一。盆地北部高岭土矿化普遍且强烈,具有很好的找矿远景。本文初步探讨了庐枞盆地高岭土成矿规律、矿床成因及找矿方向,提出了下一步开发利用的建议。 相似文献
962.
云南地区地震序列分类的定量讨论 总被引:1,自引:0,他引:1
本文通过对云南地区1965提以来116次大小地震序列的清理和归纳,引入了地震序列分类的时空强定量尺度,提出;表明震源区进人失稳状态的前震序列主要发生在主震前10天,前震序列的最大震级5.5级;震群型地震序列在时间、地点上的确定应与震级有关,在时间上以同在地震孕期内为宜,7、6、5级分别不超过1年、半年、3个月,在地点上以同在地震孕震区内为2,7、6、5级分别不超过100、50、30公里,震级上以小子等于0.5级为宜;主余震地震序列和孤立型地震序列的最大震级差分别是2.9级和3.3级 相似文献
963.
964.
A lunar occultation (LO) technique in the near-infrared (NIR) provides angular resolution down to milliarcseconds for an occulted source, even with ground- based 1 m class telescopes. LO observations are limited to brighter objects because they require a high signal-to-noise ratio (S/N ~40) for proper extraction of angular diameter values. Hence, methods to improve the S/N ratio by reducing noise using Fourier and wavelet transforms have been explored in this study. A sample of 54 NIR LO light curves observed with the IR camera at Mt Abu Observatory has been used. It is seen that both Fourier and wavelet methods have shown an improvement in S/N compared to the original data. However, the application of wavelet transforms causes a slight smoothing of the fringes and results in a higher value for angular diameter. Fourier transforms which reduce discrete noise frequencies do not distort the fringe. The Fourier transform method seems to be effective in improving the S/N, as well as improving the model fit, particularly in the fainter regime of our sample. These methods also provide a better model fit for brighter sources in some cases, though there may not be a significant imorovement in S/N. 相似文献
965.
Long‐term photometry of three active red giants in close binary systems: V2253 Oph,IT Com and IS Vir
K. Olh A. Mor K.G. Strassmeier T. Borkovits T. Granzer 《Astronomische Nachrichten》2013,334(7):625-637
We present and analyze long‐term optical photometric measurements of the three active stars V2253 Oph, IT Com and IS Vir. All three systems are single‐lined spectroscopic binaries with an early K giant as primary component but in different stages of orbital‐rotational synchronization. Our photometry is supplemented by 2MASS and WISE near‐IR and mid‐IR magnitudes and then used to obtain more accurate effective temperatures and extinctions. For V2253 Oph and IT Com, we found their spectral energy distributions consistent with pure photospheric emission. For IS Vir, we detect a marginal mid‐IR excess which hints towards a dust disk. The orbital and rotational planes of IT Com appear tobe coplanar, contrary to previous findings in the literature. We apply a multiple frequency analysis technique to determine photometric periods, and possibly changes of periods, ranging from days to decades. New rotational periods of 21.55±0.03 d, 65.1±0.3 d, and 23.50±0.04 d were determined for V2253 Oph, IT Com, and IS Vir, respectively. Splitting of these periods led to tentative detections of differential surface rotations of δP/P ≈ 0.02 for V2253 Oph and 0.07 for IT Com. Using a time‐frequency technique based on short‐term Fourier transforms we present evidence of cyclic light variations of length ≈ 10 yr for V2253 Oph and 5–6 yr for IS Vir. A single flip‐flop event has been observed for IT Com of duration 2–3 yr. Its exchange of the dominant active longitude had happened close to a time of periastron passage, suggesting some response of the magnetic activity from the orbital dynamics. The 21.55‐d rotational modulation of V2253 Oph showed phase coherence also with the orbital period, which is 15 times longer than the rotational period, thus also indicating a tidal feedback with the stellar magnetic activity. (© 2013 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献
966.
967.
地震波形分类技术在识别和划分岩相的应用中有其独特的优点,但也存在一定的局限性。通过针对不同岩相的大量实践,深入探讨了影响该技术的应用条件,系统总结了该技术识别岩相的适用性和局限性。研究表明:时窗类型及大小、地震属性体的选择是影响波形分类结果最重要的因素;不同的岩相在地震振幅、频率、相位、时间厚度上存在差异性是正确应用波形分类方法的前提;当岩相问的地震响应差别不明显,或同一岩相横向波形变化较快,无法建立统一的岩相地震波形特征时,波形分类方法的结果不能准确地划分岩相,也没有明确的地质意义。回归到岩相地震响应特点的分析,建立地震响应与岩相的对应关系,开展波形分类技术应用的先验性研究,是成功应用该技术的基础和关键。 相似文献
968.
The Late Cretaceous ükapili Granitoid including mafic microgranular enclaves intruded into metapelitic and metabasic rocks, and overlain unconformably by Neogene ignimbrites in the Ni de area of Turkey. It is mostly granite and minor granodiorite in composition, whereas its enclaves are dominantly gabbro with a few diorites in composition. The ükapili Granitoid is composed mainly of quartz, K-feldspar, plagioclase, biotite, muscovite and minor amphibole while its enclaves contain mostly plagioclase, amphibole, minor pyroxene and biotite. The ükapili Granitoid has calcalkaline and peraluminous (A/CNK= 1.0-1.3) geochemical characteristics. It is characterized by high LILE/HFSE and LREE/HREE ratios ((La/Lu) N = 3-33), and has negative Ba, Ta, Nb and Eu anomalies, resembling those of collision granitoids. The ükapili Granitoid has relatively high 87Sr/86Sr (i) ratios (0.711189-0.716061) and low εNd (t) values (-5.13 to -7.13), confirming crustal melting. In contrast, the enclaves are tholeiitic and metaluminous, and slightly enriched in LILEs (K, Rb) and Th, and have negative Ta, Nb and Ti anomalies; propose that they were derived from a subduction-modified mantle source. Based on mineral and whole rock chemistry data, the ükapili granitoid is H-(hybrid) type, post-collision granitoid developed by mixing/mingling processes between crustal melts and mantle-derived mafic magmas. 相似文献
969.