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931.
932.
An unusual timing and spectral state of a black hole microquasar XTE J1550-564 observed with RXTE is analyzed. Millisecond variabilities are found, which are significantly shorter than the minimum possible time scale in the light curves of black hole binaries, as suggested by Sunyaev & Revnivtsev (2000). The X-ray spectral fitting result indicates that there is an unusual soft component in the spectrum, which may be responsible for the millisecond variabilities. The millisecond variabilities as well as the unusual soft spectral component should be produced from some small, but independent active regions in the accretion disk. 相似文献
933.
Flare-induced signals in polarization measurements which were manifested as apparent polarity reversal in magnetograms have been reported since 1981. We are motivated to further quantify the phenomenon by asking two questions: can we distinguish the flare-induced signals from real magnetic changes during flares, and what we can learn about flare energy release from the flare-induced signals? We select the X2.6 flare that occurred on 2005 January 15, for further study. The flare took place in NOAA active re-gion (AR) 10720 at approximately the central meridian, which makes the interpretation of the vector magnetograms less ambiguous. We have identified that flare-induced signals during this flare appeared in six zones. The zones are located within an average distance of 5 Mm from their weight center to the main magnetic neutral line, have an average size of (0.6±0.4)×1017 cm2, duration of 13±4 min, and flux density change of 181±125 G in the area of reversed polarity. The following new facts have been revealed by this study: (1) the flare-induced signal is also seen in the transverse magnetograms but with smaller magnitude, e.g., about 50 G; (2) the flare-induced signal mainly manifests itself as apparent polarity reversal, but the signal starts and ends as a weakening of flux density; (3) The flare-induced signals appear in phase with the peaks of hard X-ray emission as observed by the Ramaty High Energy Solar Spectroscopic lmager (RHESSI), and mostly trace the position of RHESSI hard X-ray footpoint sources. (4) in four zones, it takes place cotemporally with real magnetic changes which persist after the flare. Only for the other two zones does the flux density recover to the pre-flare level immediately after the flare.The physical implications of the flare-induced signal are discussed in view of its relevance to the non-thermal electron precipitation and primary energy release in the flare. 相似文献
934.
随着数字地球、数字城市研究的深入,多分辨率空间数据模型已成为GIS研究的热点之一,瓦片金字塔作为管理栅格型空间数据的有效手段更得到了广泛应用.文中分析了普通金字塔模型的缺点,在此基础上设计并实现了符合TIFF和XML标准的通用数据模型;通过应用证明了模型的实用价值. 相似文献
935.
Retrograde metamorphism played the dominant role in changing the low-field rock magnetic properties and density of 198 specimens of variably retrograded eclogites from the main borehole of the Chinese Continental Scientific Drilling Project (CCSD) and from surface outcrops in the Donghai area in the southern part of the Sulu UHP belt, China. Bulk magnetic susceptibility (κ) of unretrogressed UHP eclogite is controlled by whole-rock chemical composition and ranges from 397 to 2312 μSI with principal magnetic susceptibility carrying minerals paramagnetic garnet, omphacite, rutile and phengite. Partially retrograded eclogites show large variations in magnetic susceptibility between 804 and 24,277 μSI, with high mean magnetic susceptibility values of 4372 ± 4149 μSI caused by appreciable amounts of Fe-Ti oxide minerals such as magnetite, ilmenite and/or titanohematite produced by retrograde metamorphic reactions. Completely retrograded eclogites have lower susceptibilities of 1094 ± 600 μSI and amphibolite facies mineral assemblages lacking high magnetic susceptibility minerals. Jelínek's corrected anisotropy (Pj) of eclogites ranges from 1.001 to 1.540, and shows a positive correlation with low-field magnetic susceptibility (κ). Arithmetic mean bulk density (ρ) shows a steady decrease from 3.54 ± 0.11 g/cm3 (fresh eclogite) to 2.98 ± 0.06 g/cm3 (completely retrograded eclogite). Retrograde metamorphic changes in mineral composition during exhumation appear to be the major factor causing variations in low field magnetic susceptibility and anisotropy. Retrograde processes must be taken into account when interpreting magnetic surveys and geophysical well logs in UHP metamorphic terranes, and petrophysical properties such as density and low-field magnetic susceptibility could provide a means for semi-quantifying the degree of retrogression of eclogite during exhumation. 相似文献
936.
胶州湾东北部海域生态环境污染状况研究 总被引:4,自引:1,他引:3
根据2004年5月和2005年5月两次对胶州湾东北部海域海水的盐度、pH、溶解氧、化学需氧量、无机氮、活性磷酸盐、铜、铅、锌、镉、多环芳烃和有机氯农药以及表层沉积物中有机碳、石油烃、硫化物、铜、铅、镉、汞、多环芳烃和有机氯农药测定结果,并结合2001年以来历史资料,对胶州湾东北部海域生态环境质量历史变化趋势进行了分析,该海域生态环境中除个别要素如活性磷酸盐、铅、镉、汞等重金属含量有所增加外,其他污染要素含量相对稳定且有下降趋势,2001—2005年该海域生态环境质量相对稳定,仅部分要素有加重趋势。 相似文献
937.
藏西班公湖斑岩铜矿带成矿斑岩地球化学及Pb、Sr、Nd同位素特征 总被引:9,自引:1,他引:8
对班公湖铜矿带2个具有代表性的斑岩铜矿床--多不杂铜矿床和尕尔穷铜矿床进行了详细的岩石地球化学和Pb、Sr、Nd同位素特征研究表明,与冈底斯铜矿带相比,该铜矿带含矿斑岩大离子不相容元素的富集程度相对减弱,而高场强元素和重稀土元素的亏损程度明显减轻,轻、重稀土元素的分馏程度减弱,且具有Eu的弱正异常,岩石在氧化性上更强一些;从Pb、Sr、Nd同位素特征来看,班公湖铜矿带含矿斑岩更富含放射性成因铅,~(143)Nd/~(144)Nd比值明显降低,其源区更接近印度洋沉积物区域,表明该铜矿带含矿斑岩的岩浆源区更浅,有更多的地壳物质加入;班公湖铜矿带含矿斑岩形成的构造环境属于活动大陆边缘区域,而冈底斯铜矿带明显偏离了活动大陆边缘区域,表明班公湖斑岩铜矿带形成于碰撞后地壳隆升阶段,而冈底斯铜矿带则形成于碰撞后地壳伸展阶段. 相似文献
938.
西藏班公湖岛弧带含硫化镍超基性岩的源区性质与基底背景 总被引:5,自引:1,他引:4
青藏高原班公湖一怒江成矿带上的超基性岩型硫化镍矿化是近年来在西藏地区发现的矿化新类型.文章根据成矿带西段班公湖地区含镍超基性岩体的岩石地球化学和Sr、Pb同位素分析结果,论述了含镍超基性岩浆的源区性质及生成条件,并根据锆石U-Pb LA-ICP-MS年龄测定结果,探讨了藏西北地区的基底背景.研究发现,班公湖地区的含镍超基性岩体以富集大离子不相容元素Rb、Th、U、Sr、Pb,亏损Ba、K为特点,高场强元素亏损Nb、Ti,富集Ta;稀士元素相对球粒陨石亏损强烈,但轻稀土元素相对富集.这些特点一致反映出含矿岩浆产生于受俯冲沉积物熔体交代的富集型岩石圈地幔源区.岩浆的生成深度较浅,为尖晶石二辉橄榄岩相,源区部分熔融程度较低,大体在10%左右.岩石中集中出现一批24.79亿年的残留锆石年龄,标志着当时班公湖中特斯洋盆沉积物的物源区较为单一,主要来自太古代末-元古代初的古老基底,并且推测太古代与元古代之交(25亿年)有可能是藏西北的一个古陆壳快速生长期. 相似文献
939.
西藏西部与班公湖特提斯洋盆俯冲相关的火成岩年代学和地球化学 总被引:32,自引:1,他引:31
对青藏高原西北部班公湖缝合带开展了野外地质调查,初步查明区内缝合带至少包含日土和狮泉河-改则两条蛇绿岩带。在两条蛇绿岩带北侧发现各有两期岛弧型岩浆岩发育,且形成时间严格对应。岩石地球化学分析表明,班公湖缝合带岛弧型岩浆岩的共同特征是富集大离子不相容元素Rb、Th、K和Pb;强烈亏损高场强元素Nb、Ta和Ti;Ba在微量元素蛛网图中总是相对亏损,这些特征说明班公湖地区存在两条俯冲带。从演化序列看,俯冲初期岩石属中钾钙碱性系列,之后岛弧岩浆作用向高钾钙碱性系列演变。锆石U—PbLA—ICPMS定年结果表明,北面的日土俯冲带洋壳俯冲从辉长岩墙开始,时代为(165.5±1.9)Ma(MSWD=1.16),在159Ma时岛弧岩浆作用规模增大,形成小型的花岗岩基;南面的狮泉河-改则俯冲带一开始俯冲((166.4±2.0)Ma,MSWD=3.0)就有较大规模的石英闪长岩体侵入,之后岩浆作用减弱,到159.4Ma时只有一些小体积的花岗斑岩和闪长玢岩侵入。根据岛弧岩浆作用规模,认为班公湖中特提斯洋盆的俯冲一开始是以狮泉河俯冲带为主,之后狮泉河俯冲带的俯冲作用逐渐减弱。到晚侏罗世初(159Ma)北面的日土俯冲带成为洋壳俯冲的主体。鉴于两条岛弧火成岩带在空间配置上都位于由基性-超基性岩构成的蛇绿岩带北侧,地球化学上显示陆缘弧特征,因此,认为班公湖中特提斯洋盆应该是在中侏罗世晚期(约166Ma)沿日土和狮泉河两条俯冲带同时向北俯冲,构造属性上可能不是一个统一的大洋,而是包含了多个局限性洋盆。 相似文献
940.