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2011年7月29日山西大暴雨过程的多尺度特征 总被引：1，自引：0，他引：1
利用1°×1°的NCEP再分析资料、红外辐射亮温（TBB）、多普勒雷达和气柱水汽总量等资料,对2011年7月28-29日发生在山西境内的区域性暴雨进行多尺度特征分析。结果表明：（1）乌拉尔山阻高崩溃,西风槽东移、副高进退是此次暴雨发生的环流特征;（2）850 hPa低涡切变和700 hPa暖式切变线及地面冷锋是暴雨发生的中α尺度触发系统;（3）〉30 dBZ的雷达回波呈南北向位于地面冷锋与700 hPa切变线之间,雷达回波随地面冷锋和700 hPa切变线的东移而东移;（4）低空低涡切变受500 hPa强盛西南气流的引导向东北移动,暴雨落区始终与低涡切变相伴随;（5）暴雨过程山西境内共有9个中β尺度对流云团活动,山西西南部的暴雨主要由5个中β尺度对流云团的相继移入并在自动站极大风速风场切变线附近触发对流发展所致;山西东南部的大暴雨则是3个中β尺度对流云团合并发展的结果,中γ尺度气旋是导致局地大暴雨发生的直接影响系统;（6）暴雨发生在气柱水汽总量空间分布图中水汽锋的南部和东部及靠近气柱水汽总量的大值区一侧,水汽锋的形成比降水开始提前17 h,比暴雨发生提前24 h以上,对暴雨的短期、短时预报有指示意义。 相似文献
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For the mechanism of production of γ-ray bursts (GRBs) it is rather generally recognized that the long-term γ-ray burst (LGRB) originates from the deaths of massive stars while the short-term γ-ray burst (SGRB) originates from the merging of close binaries. Therefore the speculation naturally follows that the number of LGRBs is directly proportional to the star formation rate (SFR). However, it is indicated from recent data analyses that this speculation does not fit the observations very well. It is considered that only massive stars with masses greater than a certain critical mass can produce the LGRB, so the initial mass function (IMF) of stars can significantly affect the production rate of LGRBs. In this paper it is considered that the IMF of stars can be used to explain the observed number distribution of the LGRBs with the redshift, and this has led to some good results. 相似文献
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Black holes are extremely dense and compact objects from which light cannot escape. There is an overall consensus that black holes exist and many astronomical objects are identified with black holes. White holes were understood as the exact time reversal of black holes, therefore they should continuously throw away material. It is accepted, however, that a persistent ejection of mass leads to gravitational pressure, the formation of a black hole and thus to the “death of while holes”. So far, no astronomical source has been successfully tagged a white hole. The only known white hole is the Big Bang which was instantaneous rather than continuous or long-lasting. We thus suggest that the emergence of a white hole, which we name a ‘Small Bang’, is spontaneous - all the matter is ejected at a single pulse. Thus, unlike black holes, white holes cannot be continuously observed rather their effect can only be detected around the event itself. γ-ray bursts are the most energetic explosions in the universe. Long γ-ray bursts were connected with supernova eruptions. There is a new group of γ-ray bursts, which are relatively close to Earth, but surprisingly lack any supernova emission. We propose identifying these bursts with white holes. White holes seem like the best explanation of γ-ray bursts that appear in voids. We also predict the detection of rare gigantic γ-ray bursts with energies much higher than typically observed. 相似文献
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基于滨海核电站海上γ辐射剂量率的智能化自动监测系统是一种无人值守的辐射监测装备,可全天候、长时间、在线组网、连续自动测量水面和空气中的γ剂量率、获取水中γ能谱数据并进行核素识别和计算活度浓度,并实时地将监测数据通过无线通信链路和北斗短报文两种形式上传至地面数据服务中心。在非事故情况下,该系统是对核电厂监督性监测系统的重要补充和完善;在发生重大核安全事故或放射性物质泄漏的情况下,能够有效解决传统的派船巡测时方法不标准、数据不及时不连续、人员受照风险大、船只易受污染和行动代价高等问题;在恶劣的极端气象条件下,无人值守的自动监测系统能够为核电站提供实时有效的水体和空气中的γ剂量率、气象、海水温度等监测数据,有效地提升了核电站在极端气象条件下的监测能力,对滨海核电站整体的安全性和可靠性具有一定积极意义。 相似文献
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从探伤机工作原理、有关标准规范、辐射环境影响等方面,结合某企业γ射线探伤机周围空气比释动能率实测数据,分析评价了射线探伤机使用过程中对周围环境的辐射影响程度和影响范围,提出相应的辐射安全管理及辐射防护措施。 相似文献