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1.
内蒙古陈巴尔虎旗四五牧场金矿与侏罗-白垩纪浅成-超浅成岩体关系密切,构造-岩浆热液在上侵过程中萃取部分基底岩系中的成矿物质,并在粗安质隐爆角砾岩中富集成矿。硫同位素分析表明部分成矿物质来源于围岩,包体测温表明成矿热液为低温热液,同位素测年结果表明成矿期在晚侏罗世-早白垩世。矿床为赋存于粗安质火山岩中、与侏罗-白垩纪火山-次火山活动有关的HS型浅成中低温热液型铜金矿。正磁异常区的低-负磁带状异常是矿化蚀变带的反映。具有一定规模、有明显浓集中心、浓度分带好、具明显分带的As-Sb-Ag-Hg-Au组合异常,伴有Cu,Pb,Zn,Bi异常,是寻找该类型铜金矿床的有利地段。 相似文献
2.
We present photometric observations of two post-common-envelope stars, NY Vir (=PG 1336-018) and HS 0705 + 6700. The V band CCD observation of NY Vir was performed by a 40 cm telescope at Ege University Observatory and the R band observations of HS 0705 + 6700 were performed by 100 cm telescope at TÜB?TAK National Observatory. The new light curves were analyzed by the WD code and the physical parameters of stars were determined. We obtained new mid-eclipse timings for HS 0705 + 6700 and combined them with those previously published data. The analysis of the O-C residuals yields a period of about 8.06 ± 0.28 yr and an amplitude of 98.5 s for the system HS 0705 + 6700, which is attributed to the third star physically bounded to the evolved eclipsing pair. A mass function of 1.2 × 10−4 M⊙ for the third star is obtained. The existence of a third star is also confirmed by the light curve analysis, indicating light contribution of about 0.043 at phase 0.25 in R-bandpass of the eclipsing pair. Using mass-luminosity relationship of the low mass stars we estimate a mass of 0.12 M⊙ with an orbital inclination of about 20°. The O-C residuals obtained for the system NY Vir were represented by a downward parabola which indicates orbital period decrease in the system. Using the coefficient of quadratic term we calculate a rate of orbital period decrease of about dP/dt = −4.09 × 10−8days yr−1. The period decrease we have measured in NY Vir may be explained by angular momentum loss from the binary system. 相似文献
3.
U. Bastian 《Astronomische Nachrichten》1993,314(1):39-41
Todoran's (1992) postulate of apsidal motion to explain the observed minimum times of HS Her is shown to be physically inconsistent. Instead, a third body in the system is postulated. Minimum timings in the next few years can settle the matter. 相似文献
4.
C. Simon Jeffery 《Journal of Astrophysics and Astronomy》2005,26(2-3):261-271
Subdwarf B stars play a significant role in close binary evolution and in the hot star content of old stellar populations,
in particular in giant elliptical galaxies. While the question of their origin poses several problems for stellar evolution
theory, one of their most fascinating properties is the presence of multi-periodic 2–3 minute oscillations. Interpreting these
oscillations optimally requires the correct identification of the modes. Partial identifications can be obtained using high-speed
observations of radial velocity and colour variations. We review some of the several attempts to make such observations, most
recently with the Multi-Site Spectroscopic Telescope campaign and withULTRACAM. 相似文献
5.
6.
Conflicting sorption coefficients for ortho‐phenylphenol (OPP) have been reported in the literatures, which resulted in the conflicting assessments on OPP mobility in soil. To ascertain the sorption coefficient of OPP, batch experiments were performed based on OECD guideline 106, using three types of soils. Headspace solid‐phase microextraction (HS‐SPME) and GC‐MS were applied to the determination of OPP concentration in the liquid phase. The sorption isotherms obtained for all three soils under equilibrium conditions were described well, assuming linear sorption. The organic carbon normalized distribution coefficients (Koc) ranged from 894 to 1703 L kg?1, which suggested that OPP is moderately mobile in soil. The results also showed that the Koc value of OPP can be predicted precisely from Kow, whereas it was underestimated by one order of magnitude when water solubility is used. 相似文献
7.
M. D. Reed J. R. Eggen A.-Y. Zhou D. M. Terndrup S. L. Harms D. An M. A. Hashier 《Monthly notices of the Royal Astronomical Society》2006,369(3):1529-1536
We continue our programme of extended single-site observations of pulsating subdwarf B (sdB) stars and present the results of extensive time-series photometry to resolve the pulsation spectra for use in asteroseismological analyses. PG 0154+182, HS 1824+5745 and HS2151+0857 were observed at the MDM Observatory during 2004 and 2005. Our observations are sufficient to resolve the pulsations of all three target stars. We extend the number of known frequencies for PG 0154+182 from one to six, confirm that HS 1824+5745 is a monoperiodic pulsator and extend the number of known frequencies to five for HS 2151+0857. We perform standard tests to search for multiplet structure, measure amplitude variations as pertains to stochastic excitation and examine the mode density to constrain the mode degree ℓ. 相似文献
8.
UBV light-curves of the eclipsing binary HS Herculis, obtained in 2002–2003 observational seasons, were analysed with Wilson-Devinney computer code. New absolute dimensions of the system were calculated using the results of the light-curve analysis. Period variation of the system was also investigated. Several new times of minima have been secured for this problematic system. An apsidal motion with a period of 80.7 years was confirmed and a third body in a pretty eccentric orbit (e
3 = 0.90 ± 0.08) with a period of 85.4 years was found. The corresponding internal structure constants of the binary system, log k
2, and the mass of the third body were derived. 相似文献
9.
国产HS02型湿敏电容湿度传感器性能分析 总被引：3，自引：0，他引：3
采取同球比对施放方式,选择瑞士SNOWWHITE露点式湿度探空仪作为比对标准,使用29次同球比对数据,分白天与夜间,利用随高度变化、温度分段,以及高度、温度与湿度综合分段3种方法,对大桥HS02型湿度传感器进行评估。结果表明:(1)与国外先进湿度测量仪器相比,大桥HS02型湿度传感器在准确性与稳定性方面还存在一定差距,特别表现在低温性能方面;(2)除了白天20℃以上与-30℃以下温度段大桥HS02型湿度探测偏干外,其他均呈偏湿状态,夜间所有湿度段均呈偏湿状态;(3)大桥HS02型湿度探测基本上呈现中间湿度段随机误差偏大,而两端逐渐减小的趋势,近似于">"字型变化。 相似文献
10.
Linh Hoang Elliot M. Schneiderman Karen E.B. Moore Rajith Mukundan Emmet M. Owens Tammo S. Steenhuis 《水文研究》2017,31(12):2226-2243
Saturation‐excess runoff is the major runoff mechanism in humid well‐vegetated areas where infiltration rates often exceed rainfall intensity. Although the Soil and Water Assessment Tool (SWAT) is one of the most widely used models, it predicts runoff based mainly on soil and land use characteristics, and is implicitly an infiltration‐excess runoff type of model. Previous attempts to incorporate the saturation‐excess runoff mechanism in SWAT fell short due to the inability to distribute water from one hydrological response unit to another. This paper introduces a modified version of SWAT, referred to as SWAT‐Hillslope (SWAT‐HS). This modification improves the simulation of saturation‐excess runoff by redefining hydrological response units based on wetness classes and by introducing a surface aquifer with the ability to route interflow from “drier” to “wetter” wetness classes. Mathematically, the surface aquifer is a nonlinear reservoir that generates rapid subsurface stormflow as the water table in the surface aquifer rises. The SWAT‐HS model was tested in the Town Brook watershed in the upper reaches of the West Branch Delaware River in the Catskill region of New York, USA. SWAT‐HS predicted discharge well with a Nash‐Sutcliffe Efficiency of 0.68 and 0.87 for daily and monthly time steps. Compared to the original SWAT model, SWAT‐HS predicted less surface runoff and groundwater flow and more lateral flow. The saturated areas predicted by SWAT‐HS were concentrated in locations with a high topographic index and were in agreement with field observations. With the incorporation of topographic characteristics and the addition of the surface aquifer, SWAT‐HS improved streamflow simulation and gave a good representation of saturated areas on the dates that measurements were available. SWAT‐HS is expected to improve water quality model predictions where the location of the surface runoff matters. 相似文献