排序方式： 共有53条查询结果，搜索用时 31 毫秒
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南三河沉管是鉴江供水枢纽工程中的一处跨海管道工程,管道基槽开挖会对周围海域水质产生影响。基于建立的二维非稳态水环境数学模型,利用同步水文水质监测数据对模型参数进行率定,并反演得到SS源强浓度,继而预测施工期SS对海域水环境的影响范围及程度。结果表明:距基槽中心50 m范围的SS源强浓度达到70 mg/L;SS会对基槽中心线上下游各700 m范围内的水域产生影响(增量≥10 mg/L),影响程度以挖槽为中心线向两侧递减。 相似文献
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日本鬼鲉蜇伤与P物质和生长抑素的关系及其粗毒对免疫细胞活性影响 总被引：1，自引：0，他引：1
１９９７年６月在山东省日照市岚山头附近海域收集日本鬼ｙｏｕ,采用放射凤学方法检测了注射毒腺粗提物大鼠局部肌肉组织、血浆、疹髓、延髓、中脑、下丘脑及免疫器官内Ｐ物质和生长抑素含量变化;用ＭＴＴ法检测了朱粗提物在整体和离体条件下对免疫细胞活性的影响;用生化方法检测了毒腺组织中透明质酸酶活性。结果表明,与对照组大鼠相比,实验组大鼠局部肌肉及延髓、中脑、胸腺中脾脏中Ｐ物质含量增加,而下丘脑中Ｐ物质含量下降 相似文献
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Peter J. Wheatley Christopher W. Mauche Janet A. Mattei 《Monthly notices of the Royal Astronomical Society》2003,345(1):49-61
We present the most complete multiwavelength coverage of any dwarf nova outburst: simultaneous optical, Extreme Ultraviolet Explorer and Rossi X-ray Timing Explorer observations of SS Cygni throughout a narrow asymmetric outburst. Our data show that the high-energy outburst begins in the X-ray waveband 0.9–1.4 d after the beginning of the optical rise and 0.6 d before the extreme-ultraviolet rise. The X-ray flux drops suddenly, immediately before the extreme-ultraviolet flux rise, supporting the view that both components arise in the boundary layer between the accretion disc and white dwarf surface. The early rise of the X-ray flux shows that the propagation time of the outburst heating wave may have been previously overestimated.
The transitions between X-ray and extreme-ultraviolet dominated emission are accompanied by intense variability in the X-ray flux, with time-scales of minutes. As detailed by Mauche & Robinson, dwarf nova oscillations are detected throughout the extreme-ultraviolet outburst, but we find they are absent from the X-ray light curve.
X-ray and extreme-ultraviolet luminosities imply accretion rates of 3 × 1015 g s−1 in quiescence, 1 × 1016 g s−1 when the boundary layer becomes optically thick, and ∼1018 g s−1 at the peak of the outburst. The quiescent accretion rate is two and a half orders of magnitude higher than predicted by the standard disc instability model, and we suggest this may be because the inner accretion disc in SS Cyg is in a permanent outburst state. 相似文献
The transitions between X-ray and extreme-ultraviolet dominated emission are accompanied by intense variability in the X-ray flux, with time-scales of minutes. As detailed by Mauche & Robinson, dwarf nova oscillations are detected throughout the extreme-ultraviolet outburst, but we find they are absent from the X-ray light curve.
X-ray and extreme-ultraviolet luminosities imply accretion rates of 3 × 10
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《Astroparticle Physics》2009,32(2):112-119
SS433, located at the center of the supernova remnant W50, is a close proximity binary system consisting of a compact star and a normal star. Jets of material are directed outwards from the vicinity of the compact star symmetrically to the east and west. Non-thermal hard X-ray emission is detected from lobes lying on both sides. Shock accelerated electrons are expected to generate VHE gamma rays through the inverse-Compton process in the lobes. Observations of the western X-ray lobe region of SS433/W50 system have been performed to detect VHE gamma rays using the 10 m CANGAROO-II telescope in August and September, 2001, and July and September, 2002. The total observation times are 85.2 h for ON source, and 80.8 h for OFF source data. No significant excess of VHE gamma rays has been found at three regions of the western X-ray lobe of SS433/W50 system. We have derived 99% confidence level upper limits to the fluxes of gamma rays and have set constraints on the strengths of the magnetic fields assuming the synchrotron/inverse-Compton model for the wide energy range of photon spectrum from radio to TeV. The derived lower limits are G for the center of the brightest X-ray emission region and G for the far end from SS433 in the western X-ray lobe. In addition, we suggest that the spot-like X-ray emission may provide a major contribution to the hardest X-ray spectrum in the lobe. 相似文献
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曲线顶管施工技术以其特有的优势和应用领域,越来越受到重视。总结了国际上常用的曲线顶管施工技术,分别以SS MOLE和Ultimate Method两种具有代表性的工法为例介绍了曲线顶管技术的地层适应性、适用管道直径、应用领域和所能达到的最小曲率半径。对曲线顶管施工中顶进力计算这一重点和难点,给出了曲线顶管顶推力计算公式,并举例说明了曲线段顶推力计算公式的实际应用。 相似文献
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本文通过合成SH波理论地震图的方法,利用SS-S走时和SS波波形资料,研究了我国上地幔剪切波速度结构。初步结果表明,我国大陆上地幔可以分成两个独立不同的速度结构模型:一是青藏高原;另一是中国大陆东部。两部分均存在剪切波低速层,但埋藏深度不同,高原部分是100km,东部地区是60km,两部分的差异大约在350km以下趋于消失。在405km和660km深处存在剪切波的速度间断面。400km以下青藏高原和中国大陆东部地区剪切波的速度结构与北美洲、北大西洋西部、欧洲、阿尔卑斯带地区的结构一致,说明在这几个地区上地幔剪切波速度结构的横向变化在400km以下很小。 相似文献
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利用国家测震台网固定台站和“中国地震科学台阵探测”项目在南北地震带北段布设的宽频带流动台阵记录到的极远震事件,通过SS前驱波震相研究,获得了阿留申—阿拉斯加俯冲带东段及邻区下方410 km和660 km间断面的埋深和起伏形态特征.为增强对SS前驱波震相的识别,我们采用了时差校正和共反射点叠加分析.叠加结果显示,毗邻阿留申俯冲带的白令海、阿拉斯加半岛、以及阿拉斯加中南部和东部地区下方,410 km和660 km间断面的埋深基本呈正相关关系,因而具有正常的过渡带厚度.这表明在阿留申—阿拉斯加俯冲带东段,北太平洋板块还没有俯冲到地幔过渡带深度范围内.其次,在阿拉斯加西部地区下方,660 km间断面出现明显下沉,而上覆的410 km间断面埋深接近于全球平均值,从而导致过渡带明显加厚.据此,我们推测在阿拉斯加西部地区下方地幔过渡带底部可能存在库拉残留板块. 相似文献
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考虑超随机特性的人工地震动合成 总被引：5，自引：5，他引：0
文中根据自相关函数随机噪声部分的2个重要性质提出了自相关函数随机噪声部分的迭代生成算法,并给出了以确定性自相关函数为目标函数,考虑随机噪声部分影响的人工合成地震动方法.本文的研究结果表明地震动加速度的平方和（SS）比峰值加速度（PGA）更好地量度了地震地面运动强度.文中用蒙特卡罗方法分析了自相关函数噪声项对人工合成地震动幅值和反应谱的影响：由于自相关函数的随机噪声项对地震动总功率或平方和的贡献为0,因此随机噪声项对合成地震动幅值的影响不大,但由于自相关函数随机噪声项明显改变了地震动功率谱在频域上的分布特征,使原本光滑的平均反应谱出现了明显的波动,从而在一定程度上提高了平均反应谱的峰值,使自相关函数噪声部分对平均反应谱也有一些影响. 相似文献