基于地磁参数和子午线收敛角计算的井斜方位角校正方法          下载免费PDF全文

林彦兵  闫吉曾 《探矿工程》2012,39(12):11-14

井斜方位角的校正对于定向井轨迹控制、中靶分析有非常重要的意义。通过分析大地坐标与高斯克吕格投影坐标之间的关系,根据地磁场球谐函数模型,地磁参数和子午线收敛角的计算模型,提出了实现方式和求解步骤,并编制了相应的计算软件。通过实例计算与分析,表明地磁参数和子午线收敛角的准确计算对于定向井轨迹控制的重要性。  相似文献   

Distribution of local Cs anomalies on the seafloor near the Fukushima Dai-ichi Nuclear Power Plant     

Blair Thornton  Seiki Ohnishi  Tamaki Ura  Naoteru Odano  Shun Sasaki  Tsuneo Fujita  Tomowo Watanabe  Kaoru Nakata  Tsuneo Ono  Daisuke Ambe 《Marine pollution bulletin》2013

An estimated 3.5 ± 0.7 × 10¹⁵ Bq of ¹³⁷Cs is thought to have been discharged into the ocean following the melt down at Fukushima Dai-ichi Nuclear Power Plant (F1NPP). While efforts have been made to monitor seafloor radiation levels, the sampling techniques used cannot capture the continuous distribution of radionuclides. In this work, we apply in situ measurement techniques using a towed gamma ray spectrometer to map the continuous distribution of ¹³⁷Cs on the seafloor within 20 km of the F1NPP. The results reveal the existence of local ¹³⁷Cs anomalies, with levels of ¹³⁷Cs an order of magnitude higher than the surrounding seafloors. The sizes of the anomalies mapped in this work range from a few meters to a few hundreds of meters in length, and it is demonstrated that the distribution of these anomalies is strongly influenced by meter scale features of the terrain.  相似文献   

沈阳地震台大震速报震级差分析     

包秀敏  马莉  顾强强  梁一婧 《防灾减灾学报》2013,(3):64-67

利用沈阳台测算震级与国家台网速报标准震级进行比较,寻找存在震级差的原因,分析得出,台站测算震级存在误差的原因主要有震中距,方位角,地震震级等。  相似文献   

内蒙古四子王旗芒和特铀矿地质特征     

李宝辉 《国外铀金地质》2012,(1):27-30

在铀矿航空γ能谱测量和地面放射性普查工作的基础上,通过对铀矿异常进行地表揭露和钻探工程验证,发现了芒和特铀矿床。铀矿床类型为湖沼相砂岩型沉积矿床,含铀矿岩石为古近系粉砂岩,铀矿化具有放射性强度较弱、铀含量较高和矿化分布不均匀的特点。深入分析铀矿放射性强度弱的原因,采用放射性测量结合化学样品分析的方法,能够提高找矿效率。  相似文献   

Effect of resonant neutrino oscillation on TeV neutrino flavor ratio from choked GRBs     

Sarira Sahu 《中国天文和天体物理学报》2010,10(10)

In the collapsar scenario of the long duration Gamma-Ray Bursts (GRBs),multi-TeV neutrino emission is predicted as the jet makes its way through the stellar envelope.Such a neutrino signal is also expected for more general failed GRBs in which a putative jet is choked by a heavy envelope.If the ν e →νμ neutrino oscillation parameters are in the atmospheric neutrino oscillation range,we show that the resonant oscillation of ν e  νμ,τ can take place within the inner high density region of the choked jet prog...  相似文献   

承德黑山矿区钻孔纠斜技术及防斜技术措施          下载免费PDF全文

赵均文  于志坚  邢运涛  丁国东 《探矿工程》2010,37(5):17-21

近两年,河北承德黑山矿区钻孔顶角、方位超差一直是困扰地质技术人员和钻探施工人员的一大难题,针对生产实际问题,采用LZ-73（89）造斜器进行纠偏,取得了较好的效果。此外,在分析钻孔跑偏的主要原因和总结施工经验的基础上,提出了预防钻孔偏斜的技术措施,实践证明措施科学有效。  相似文献   

Swift时代伽马射线暴的观测和理论     

林一清 《天文学进展》2011,29(2)

伽马射线暴是宇宙中最剧烈的爆发现象之一.Swift卫星的快速定位和Fermi卫星的宽、高能段观测,使得伽马暴的观测可以全波段进行.通过Swift的观测可以对伽马暴现象的本质有进一步的理解,而Fermi卫星提供了一些暴高能光子的辐射数据,为进一步研究暴的辐射机制和伽马暴以及它的余辉提供了有力的依据.介绍了Swift和Fermi卫星发射后一些伽马暴的观测和理论研究进展.  相似文献   

Present Observational Status of the Intermediate Mass Stars: δ Sct Stars, γ Dor Stars and roAp Stars     

D.W. Kurtz 《Astrophysics and Space Science》2003,284(1):29-36

The present observational status of the Sct stars, Dor stars and roAp stars is discussed. The Sct stars are the most intensively observed of the three groups, but it has become clear that there are severe problems in extracting asteroseismic information from them. Dozens of frequencies are observed, but hundreds of frequencies are predicted from the models; unique matches of observation and theory still elude us. The Sct stars are observationally complex – some recent `best case' campaigns are discussed. It is possible that substantial observational advances for Sct stars may need to await upcoming satellite missions. New Dor stars are beingdiscovered frequently, and new behaviour is being found for them. They constitutean observationally young field. Their pulsational frequency range is being expanded, their position in the HR diagram is becoming better known (but is yet to be fully constrained), and the possibility exists of hybrid Dor – Sct stars that have greatasteroseismic promise, although it is clear such stars are rare, if they do exist. It has been observationally challenging to extract more than a fewfrequencies for any Dor star so far. Exciting spectroscopic discoveries of new behaviour in roAp stars promise unprecedented information about the structure of the peculiar atmospheres ofthose stars – pulsation amplitude and phase in 3D, magnetic field structurein 3D, abundance stratification in 3D, realistic T- for the most peculiarstars – as well as entirely new information about the interaction of pulsation,rotation and magnetic fields. Recent theoretical work has led to new understandingof the previously inexplicable frequency spacing of HR 1217 with new Whole Earth Telescope observations supporting this theory. An `improved oblique pulsator model' has been developed in which the pulsationaxis is not the magnetic axis; this model has passed several observationaltests and new ones are being devised to examine it further.  相似文献   

Using X‐shooter to measure the extinction in long GRB host galaxies from emission lines     

K. Wiersema 《Astronomische Nachrichten》2011,332(3):295-296

The spectra of the host galaxies of gamma‐ray bursts at low redshift generally show strong hydrogen lines of the Balmer, Paschen and Brackett series, in addition to strong nebular metal lines. In special cases the hosts can be resolved in separate star forming regions, and spatially resolved spectroscopy can be obtained. Generally, the three strongest Balmer lines are used to derive the reddening experienced by the emission lines of the host gas, assuming a Milky Way extinction curve, case B recombination and a fixed electron temperature. We demonstrate how the wide wavelength range of X‐shooter, in combination with a rigorous calibration strategy, can be used to fit explicitly for R_V, T_e, and A_V simultaneously using a large number of H and He I recombination lines, explicitly corrected for stellar atmosphere absorption. This increases our understanding of extinction and absorption in starforming regions in GRB hosts. We use two GRB hosts as examples of the methods, outlining the advantages of using X‐shooter over other instruments (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

幂律电子谱轫致辐射积分的快速计算     

李友平  甘为群 《天文学报》2011,52(3)

SSW(Solar SoftWare)的能量电子产生X光子的轫致辐射积分计算发展到版本2时,其性能相比初始的版本1提高很多.在版本2的基础上,对这个积分进一步改进.通过对比几种轫致辐射积分方案,结果显示,最终的方案性能上比版本2可以快约2～5倍.在积分的精确性上比版本1及版本2均改进了很多,在缺省的积分控制精度下也不再产生光子谱的尖刺现象.而且,积分耗时不再敏感于积分上限取值.由于积分性能的提高,使得利用精确的轫致辐射截面计算轫致积分成为可能.结果显示,用精确轫致辐射截面比先前的近似截面积分的结果光子流量略小(≤4%),积分时间大约比先前使用近似截面多30%.  相似文献