Polarization observations of giant radio pulses from the millisecond pulsar B1937+21 at a frequency of 600 MHz

We performed polarization observations of giant radio pulses from the millisecond pulsar B1937+21. The observations were carried out in July 2002 with the 64-m Kalyazin radio telescope at a frequency of 600 MHz in two polarization channels with left-and right-hand circular polarizations (RCP and LCP). We used the S2 data acquisition system with a time resolution of 125 ns. The duration of an observing session was 20 min. We detected twelve giant radio pulses with peak flux densities higher than 1000 Jy; five and seven of these pulses appeared in the RCP and LCP channels, respectively. We found no event that exceeded the established detection threshold simultaneously in the two polarization channels. Thus, we may conclude that the detected giant pulses have a high degree of circular polarization, with the frequency of occurrence of RCP and LCP pulses being the same.     

Optimization of grid-drilling using computer simulation

A computer simulation method has been developed to find efficient drilling grids for mineral deposits. A well-known ore deposit is used as a model to develop an efficient pattern for undiscovered ore bodies in the same area or in other prospects where similar geometry is suspected. The model for this study is the Austinville, Virginia deposit, a Mississippi Valley-type deposit composed of 17 ore bodies totaling 34 million short tons (30 million metric tons). The method employs a computer program that simulates drilling the model deposit with different patterns, including various levels of follow-up drilling. Follow-up holes are drilled in fences at one half the original spacing around holes in the grid that show ore-grade mineralization. Each pattern is drilled 100 times from random starting locations to provide a range of outcomes of drilling, including the best, worst, and most likely. For this study, patterns of 100 drill holes were composed of 10 fences spaced 1000–5000 feet (305–1524 m) apart, each with 10 holes spaced 200–1000 feet (61–305 m) apart. In all, 25 grids were used with zero to three levels of follow-up drilling. The 600/2000 grid, with drill holes spaced 600 feet (183 m) apart in fences spaced 2000 feet (610 m) apart, was compared with the 200/5000 grid because they represented contrasting outcomes. The 600/2000 grid penetrated many ore bodies consistently but with few multiple hits to individual ore bodies; whereas the 200/5000 grid inconsistently penetrated few ore bodies with many multiple hits. The 600/2000 grid was more efficient than the 200/5000 grid at hitting large ore bodies of 1,000,000 short tons or greater (900,000 metric tons or greater) and was made more effective by adding one cycle of follow-up drilling. The 600/2000 grid had a 97% chance of hitting one or more large ore bodies with at least one drill hole per ore body, and the 200/5000 grid had a 64% chance. Once hit, there was an 82% chance that the largest ore body would be penetrated by three or more holes when using the 600/2000 grid and an 88% chance using the 200/5000 grid.     

Origin of short period comets

Reasons for interest in the origin of short-period comets and the difficulties of computing their long-term dynamcal evolution are reviewed. The relative advantages of a source region in an extended inner core of the Oort cloud or a compact comet belt just beyond the planetary system are finely balanced, and it is premature to consider the problem solved. A complication is that some comets belonging to the Jupiter family may be part of a time-dependent system, possibly the remains of a giant comet such as Chiron which could have been part of the system 104 yr ago. The origin of short-period comets plays a pivotal role in many areas of solar system science: planet formation, the source of water (possibly life) on the terrestrial planets, the cratering record on the terrestrial planets and satellites of the outer planets, and the environmental impact posed by massive bodies and their decay products in the Earth's near-space environment.     

云南潞西大矿山铅锌矿

矿体产于花岗岩以上断层附近大理岩中,大理岩与花岗岩接触部位是主要的矿化部位,在大矿山、小石林、灰窑等地见有强褐铁矿化、弱铅锌矿化的厚大矿化层。通过勘查工作,认为矿区具有寻找中-大型规模矿山的前景。     

大理宾川小龙潭斑岩型铜矿

矿体赋存于不同构造过渡带断裂侧,控矿岩石为喜马拉雅期浅成—超浅成相的富钾碱性系列的中酸性侵入体,属于斑岩型铜矿。     

安徽池州铜山铜矿深部找矿实践与启示

铜山铜矿资源储量日益枯竭。危机矿山接替资源勘查中,采用地质、物探综合手段圈定异常区,经深部钻探验证,取得突破。     

大岭子金矿地质特征及选矿浸出率

大岭子金矿V1矿体赋存于中元古界高黎贡山群变质岩中,受韧性剪切带控制,矿石类型以氧化矿石为主。提出选矿依据。     

富宁阳文冲-广南菜子垣热液淋滤卡林型金矿区

金矿区构造活动具有多期性：加里东期及海西期在矿区形成的薄弱角度不整合面、近南北向平行的滑脱断层,是含矿热液的运移、沉淀的通道和空间。金矿床应属地下热液淋滤卡林型金矿床。     

云南永胜宝坪浅源热液改造型铜矿地质及成因

宝坪铜矿赋存于三叠系下统腊美组中。矿体呈似层状,少量脉状,严格受北北西-北西向构造控制。矿床成因类型属浅源热液改造型铜矿床。     

普朗铜矿找矿标志及找矿模型

普朗铜矿矿体形态简单,以铜为主,伴生金、硫等多种有益组份。找矿标志为深大断裂旁侧的次级两组断裂交汇部位;特别是多种岩类的杂岩体,裂隙发育地段;斑岩体靠沟谷部位(负地形)等。土壤化探异常Cu>400×10-6和Mo>10×10-6异常叠加部位;视极化率大于10%的激电异常,磁异常约50～100nT的部位等。初步建立找矿模型,运用该模型,在矿区外围已发现普上、亚杂等一批铜(多金属)矿体,矿化体,具有明显的找矿指导意义。