北海区海洋放射性环境监测预警信息系统的设计与实现          下载免费PDF全文

张馨星  邓春梅  王伟  王荣元  魏计房  高晓慧 《应用海洋学学报》2020,39(1):117-121

本研究针对海洋管理部门监测预警的需求,开发了北海区海洋放射性环境监测预警信息系统。系统主要由信息数据库、分析评价模块、信息预警模块三大部分组成。该系统实现了放射性监测数据的管理和自动化评价分析,实现了核事故的预警、应急响应时的模拟预测、信息传输、信息通报等信息化管理。系统开发完成后,在海区放射性监测航次中对部分功能进行了应用,极大的提高了工作效率,为海洋放射性监测预警工作提供了技术支持。  相似文献   

Examination of scaling between proposed early signals in P waveforms and earthquake magnitudes     

M. A. Lewis  Y. Ben-Zion 《Geophysical Journal International》2007,171(3):1258-1268

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Evolution of massive haloes in non-Gaussian scenarios     

M. Grossi  K. Dolag  E. Branchini  S. Matarrese  L. Moscardini 《Monthly notices of the Royal Astronomical Society》2007,382(3):1261-1267

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Does radiative feedback by the first stars promote or prevent second generation star formation?     

Kyungjin Ahn  Paul R. Shapiro 《Monthly notices of the Royal Astronomical Society》2007,375(3):881-908

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Probing the star formation history using the redshift evolution of luminosity functions     

Saumyadip Samui  Raghunathan Srianand  Kandaswamy Subramanian 《Monthly notices of the Royal Astronomical Society》2007,377(1):285-299

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Eccentricity cycles shown by early Pleistocene planktonic foraminifers of the Omma Formation, Sea of Japan     

Akihisa Kitamura  Katsunori Kimoto 《Global and Planetary Change》2007,55(4):273-283

There is a continuous record of planktonic foraminifers for oxygen isotope stages 50 to 26 (ca. 1.5–1.0 Ma) in the early Pleistocene Omma Formation near Kanazawa City, Central Japan, on the Sea of Japan coast. The warm-water species Globigerinoides ruber entered the Sea of Japan with the Tsushima Current during all interglacial periods and went locally extinct in the succeeding glacial periods. This implies that the marine climate of the Sea of Japan varied predominantly with the 41,000-year period of Earth's orbital obliquity. However, the relative abundances of G. ruber in marine isotope stages 47, 43 and 31 are significantly higher than those in other interglacial stages. These stages correspond to periods when eccentricity-modulated precession extremes were aligned with obliquity maxima. The Tsushima Current is a branch of the warm Kuroshio Current which is the strong northwestern component of the subtropical North Pacific Ocean gyre. Our data imply that the early Pleistocene climate in the northwestern Pacific was influenced not only by obliquity cycles but also by eccentricity cycles. This study also supports the climate model regarding eccentricity's role in the origin of low-frequency climate changes before the late Pleistocene ice ages.  相似文献   

The imprint of massive black hole formation models on the LISA data stream     

Alberto Sesana  Marta Volonteri  Francesco Haardt 《Monthly notices of the Royal Astronomical Society》2007,377(4):1711-1716

The formation, merging and accretion history of massive black holes (MBHs) along the hierarchical build-up of cosmic structures leaves a unique imprint on the background of gravitational waves (GWs) at mHz frequencies. We study here, by means of dedicated simulations of black hole build-up, the possibility of constraining different models of black hole cosmic evolution using future GW space-borne missions, such as LISA . We consider two main scenarios for black hole formation, namely, one where seeds are light (  ≃10² M_⊙  , remnant of Population III stars) and one where seeds are heavy (  ≳10⁴ M_⊙  , direct collapse). In all the models we have investigated, MBH binary coalescences do not produce a stochastic GW background, but rather, a set of individual resolved events. Detection of several hundreds merging events in a 3-yr LISA mission will be the sign of a heavy seed scenario with efficient formation of black hole seeds in a large fraction of high-redshift haloes. At the other extreme, a low event rate, about a few tens in 3 yr, is peculiar of scenarios where either the seeds are light, and many coalescences do not fall into the LISA band, or seeds are massive, but rare. In this case a decisive diagnostic is provided by the shape of the mass distribution of detected events. Light binaries  ( m < 10⁴ M_⊙)  are predicted in a fairly large number in Population III remnant models, but are totally absent in direct collapse models. Finally, a further, helpful diagnostic of black hole formation models lies in the distribution of the mass ratios in binary coalescences. While heavy seed models predict that most of the detected events involve equal-mass binaries, in the case of light seeds, mass ratios are equally distributed in the range 0.1–1.  相似文献   

Astrophysical and cosmological information from large-scale submillimetre surveys of extragalactic sources     

M. Negrello  F. Perrotta  J. González-Nuevo González  L. Silva  G. De Zotti  G. L. Granato  C. Baccigalupi  L. Danese 《Monthly notices of the Royal Astronomical Society》2007,377(4):1557-1568

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铅污染水稻的冠层高光谱特征研究   总被引：10，自引：1，他引：9  

任红艳  庄大方  潘剑君  邱冬生 《地球信息科学学报》2008,10(3):314-319

本研究通过铅污染土壤中的水稻盆钵栽培试验,考察了水稻对土壤重金属铅的吸收以及铅对水稻生长的胁迫,并借助地面高光谱辐射仪器获取多个生育期（苗期、分蘖前期、分蘖盛期、拔节期和孕穗期）的水稻冠层高光谱反射数据。在进行光谱测量的同时测定了水稻植株体内的铅含量与冠层叶片叶绿素含量。分析结果表明:铅污染胁迫下水稻冠层叶片叶绿素含量与叶绿素a、b组成变化明显,可见光区间520nm～560nm和630nm～690nm处是铅污染水稻对冠层反射高光谱敏感的特征波段。通过模拟高光谱分辨率遥感传感器MODIS的相应波段（第4通道:545nm～564nm、第1通道附近:620nm～670nm）以及考虑叶绿素的荧光特征（760nm）,本研究分别选择敏感波段中的552nm,672nm与760nm构造了复合归一化污染指数CNDPI（Compos-ite Normalized Difference Pollution Index）,分析发现CNDPI能够明显地区分不同铅污染水平的水稻。在分蘖前期采用适当的冠层光谱反射率形式（敏感波段、CNDPI）可以实现水稻铅污染的遥感监测。  相似文献   

马氏珠母贝胚胎和早期幼虫冷冻的研究   总被引：3，自引：0，他引：3  

王鹏飞  王梅芳  余祥勇 《广东海洋大学学报》2008,28(1):25-28

0～4℃下,不同发育时期的马氏珠母贝(Pinctada martensii)胚胎和幼虫在不同浓度的DMSO抗冻保护液中放置30min后,置室温恢复,并以不同浓度的DMSO作为抗冻保护液,通过缓慢降温对不同发育时期的胚胎和早期幼虫进行超低温(-196℃)冷冻、35℃水浴快速解冻。结果表明:低温下DMSO对胚胎和早期幼虫活力影响较弱;马氏珠母贝的囊胚和担轮幼虫存活率较低。当DMSO体积分数为14%时,原肠胚的存活率为10%左右,且部分胚胎能够继续发育至D形幼虫;当DMSO体积分数为14%、16%时,解冻后的D形幼虫存活率超过49.9%,其中大部分存活48h以上。  相似文献