本溪地区太古宙岩石中黑云母击象的发现及其地质意义     

崔文智 《国土资源》1989,(2)

作者在辽宁省本溪地区大范围内发现黑云母击象,这在该区尚属首次。黑云母击象以及存在的地质环境表明,在地质演变史上,本溪地区曾存在至少一期影响普遍的快速构造变形—岩浆活动事件,它很可能代表一次古断裂地震活动。  相似文献   

Long term variations in solar flare activity     

J. N. Goswami  R. Jha  D. Lal 《Journal of Astrophysics and Astronomy》1981,2(2):201-212

A statistical analysis of the contemporary (1954-1975) solar flare particle events has been made for the parametersF (integrated, proton fluence in cm^-2 in an event with kinetic energy above 10 MeV) andR ₀ (the characteristic rigidity). These data are compared with the long-term averaged values determined from stable- and radio-nuclide measurements of lunar samples. The analysis shows that the ancient solar flare proton spectrum was harder (higher R₀ values) compared to that observed in contemporary flares. A similar analysis can not be made for the mean long-term averaged flux (ˉJ, cm^-2 S^-1), since the contemporary averages suffer from an uncertainty due to the statistics of a single event. However, the average flux estimates for time durations 〈T〉 exceeding 10³ yr, are free from such uncertainties. The long-term averaged ˉJ values obtained over different time scales (10⁴ - 10⁶ yr) suggest a possible periodic variation in solar flare activity, with enhanced flux level during the last 10⁵ yr. The available data rule out the occurrence of giant flares, with proton fluence exceeding 10¹⁵ cm^-2 during the last million years.  相似文献   

1984年2月14日大角星色球活动的CaⅡ H,K线观测     

秦松年  李久康 《中国天文和天体物理学报》1987,(1)

我们用云台一米望远镜Coudé摄谱仪得到大量的大角星(αBoo)的高分辨率光谱,从中找到1984年2月14日一组随时间变化的CallH,K线光谱。经对比分析,我们认为这可能是一次大角星的色球爆发,其特征如下:在连续观测近四小时中获得5张光谱片,可看出CallH,K线轮廓的变化。它们变化的顺序是:开始出现轮廓的不对称一轮廓仍然不对称并伴随着峰值发射增强一轮廓恢复到对称状况;K_2线中K_(2V)与K_(2r)最大不对称为20％。发射极大时K_(2S2)峰值增强20％左右。K_(1r)和K_(1V)的变化也明显。特别是K_3线在K_2线峰值增强时出现吸收线反转出发射线核。  相似文献   

Organic nitrogen and caloric content of detritus: II. Microbial biomass and activity     

Roger B. Hanson 《Estuarine, Coastal and Shelf Science》1982,14(3):325-336

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太阳活动预报中的模糊识别综合指数     

张勤 《中国天文和天体物理学报》1990,(1)

在太阳活动预报中,预报因子的选取和处理对预报效果影响甚大。本文在云台原有的平均综合指数基础上,运用模糊识别方法,给出了一种模糊识别综合指数,它能更好地表征太阳日面活动区的活动特征。这种方法简单、方便,较充分地利用了预报因子中所含有的有用信息,从而使识别预报率有所提高。  相似文献   

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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十堰及邻区地震构造环境浅析     

许光炳  刘可  付燕玲  耿爱玲 《大地测量与地球动力学》2003,23(4):105-110

研究了十堰及邻区区域构造背景和地球物理场分布特点，分析了区域性地震构造与有感地震和中强地震活动的关系。结果表明：区内中强地震活动与北西西向、北北西向断裂及北东-北北东向断裂密切有关；5级左右地震活动发生在大型沉降区内次级凸起与凹陷的交接带、现代构造活动的盆地或地槽、莫霍面斜坡扭曲部位；6级以上地震发生在现代地壳隆起边缘的沉降区一侧或大型凸起与凹陷区的过渡部位。  相似文献   

秦皇岛市区断裂活动性的SEM研究     

杜东菊 《地球科学与环境学报》1989,(3)

近年来,应用断层泥扫描电子显微(SEM)构造来研究断裂的活动性,已引起了国内、外地震地质和工程地质的重视。本文通过对秦皇岛市区几条断裂带断层泥和断层泥中石英颗粒表面SEM构造特征的研究,对断裂带的相对活动时限及活动特征进行了探讨。研究成果与野外宏观调查、现场仪器测试、遥感101系统图象处理结果基本吻合,在微观领域为市区断裂活动性研究提供了依据。这说明该方法在工程地质领域具有重要的实际应用价值。  相似文献   

BV photometry of UX Arietis     

S. Mohin  A. V. Raveendran 《Journal of Astrophysics and Astronomy》1989,10(1):35-45

DifferentialBV photometry of UX Ari obtained on 58 nights during 1984-85, 1985-86, 1986-87, and 1987-88 observing season is presented. We find that (B-V) is phase dependent with the system being reddest at the light maximum and we interpret this as due to the variable fractional contribution by the G5 V component to the total light at shorter wavelengths. An analysis of the available data indicates that at larger amplitudes of the photometric wave the brightness at maximum increases and that at minimum decreases and both converge to δV ≃ −1.0 mag at very low amplitudes. It implies that the low wave amplitudes are essentially due to more homogeneity in the surface distribution of spots rather than due to low levels of spot activity. The variation in wave amplitude is found to be near-sinusoidal with a period around 13–14 years  相似文献   

FTIR Spectrum of Phenocryst Olivine as an Indicator of Silica Saturation in Magmas   总被引：3，自引：0，他引：3  

MATVEEV  S.; PORTNYAGIN  M.; BALLHAUS  C.; BROOKER  R.; GEIGER  C. A. 《Journal of Petrology》2005,46(3):603-614

Fourier Transform infrared (FTIR) absorption spectra of hydroxylwere measured on olivine phenocrysts from hydrous basaltic meltsthat originated in island-arc tectonic settings. The basalticmelts encompass a wide range of silica activities from orthopyroxene-saturatedhypersthene-normative to nepheline-normative compositions. Theintensities and wavenumber placement of hydroxyl absorptionbands correlate with the degree of silica saturation of theparent melt from which the olivine crystallized. Olivines fromsilica-undersaturated nepheline-normative melts absorb IR radiationin the wavenumber range 3430–3590 cm^–1 (Group 1).In contrast, olivines from orthopyroxene-saturated boniniticmelts exhibit hydroxyl absorption bands in the wavenumber range3285–3380 cm^–1 (Group 2). Olivines crystallizedat intermediate silica activities exhibit a combination of thetwo groups of hydroxyl IR bands, where the proportion of Group2 bands increases with increasing silica saturation of the parentmelt. The positions of hydroxyl absorption peaks observed herefor natural samples are consistent with previous measurementson experimentally annealed olivines. Thus protonation experimentscan be employed to make spectroscopically dry olivine structuresvisible by IR, yielding information on the silica saturationof the parental magmas. Hydroxyl concentrations in the studiedolivines were estimated to be 1–2 ppm, corresponding toan olivine–melt partition coefficient of (1·0 ±0·3) x 10^–4. KEY WORDS: nominally anhydrous minerals; olivine; water; mantle; silica activity; melt inclusions  相似文献