实现物探测线高效布设的一种方法

物探测线布设是一项重要的基础性工作,其施工效率直接影响物探勘查工作的开展。利用GPS相关软件完成测点数据的批量输入可以在很大程度上提高工作效率,但随着USB接口的支持及普及,其效果便不再那么明显和突出,相比之下兼容格式的研究与应用更能有效地提高测线布设的效率,也更为简便和有效。为了进一步提高工作效率,利用Visual C++编程简化了测线布设中涉及的测线计算和数据输入等操作流程,避免了手工计算和数据格式转换的麻烦,达到了测线高效布设的目的。文中详细介绍了物探弯曲测线的计算方法和常用GPS兼容格式的转换方法与软件应用。实例表明该方法方便、有效,能节省大量的室内和野外工作量。

利用无人机航测影像进行物探测线优化设计

黄土塬地区沟、塬、梁、峁等地形纵横交错,加之油田建设及地方大面积开发建设,造成地形、地物复杂,对长庆油田陇东探区地震勘探测线布设及资料采集造成了很大的困难,导致测线重复设计、采集作业效率低下、作业质量无法保证、勘探成本难以控制等问题的出现。本文介绍了利用无人机拍摄的高清影像,针对黄土塬等地形、地物复杂地区地震勘探测线优化设计进行了的探讨。

Search for gamma-ray spectral lines with the DArk Matter Particle Explorer

The DArk Matter Particle Explorer(DAMPE)is well suitable for searching for monochromatic and sharpγ-ray structures in the GeV-TeV range thanks to its unprecedented high energy resolution.In this work,we search forγ-ray line structures using five years of DAMPE data.To improve the sensitivity,we develop two types of dedicated data sets(including the BgoOnly data which is the first time to be used in the data analysis for the calorimeter-based gamma-ray observatories)and adopt the signal-to-noise ratio optimized regions of interest(ROIs)for different DM density profiles.No line signals or candidates are found between 10 and 300 GeV in the Galaxy.The constraints on the velocity-averaged cross section for xx→γγand the decay lifetime for x→γv,both at 95%confidence level,have been calculated and the systematic uncertainties have been taken into account.Comparing to the previous Fermi-LAT results,though DAMPE has an acceptance smaller by a factor of~10,similar constraints on the DM parameters are achieved and below 100 GeV the lower limits on the decay lifetime are even stronger by a factor of a few.Our results demonstrate the potential of high-energy-resolution observations on dark matter detection.

Detection of spectral hardenings in cosmic-ray boron-to-carbon and boron-to-oxygen flux ratios with DAMPE

Boron nuclei in cosmic rays(CRs)are believed to be mainly produced by the fragmentation of heavier nuclei,such as carbon and oxygen,via collisions with the interstellar matter.Therefore,the boron-tocarbon flux ratio(B/C)and the boron-to-oxygen flux ratio(B/O)are very essential probes of the CR propagation.The energy dependence of the B/C ratio from previous balloon-borne and space-based experiments can be well described by a single power-law up to about 1 TeV/n within uncertainties.This work reports direct measurements of B/C and B/O in the energy range from 10 Ge V/n to 5.6 TeV/n with 6 years of data collected by the Dark Matter Particle Explorer,with high statistics and well controlled systematic uncertainties.The energy dependence of both the B/C and B/O ratios can be well fitted by a broken power-law model rather than a single power-law model,suggesting the existence in both flux ratios of a spectral hardening at about 100 Ge V/n.The significance of the break is about 5.6σand 6.9σfor the GEANT4 simulation,and 4.4σand 6.9σfor the alternative FLUKA simulation,for B/C and B/O,respectively.These results deviate from the predictions of conventional turbulence theories of the interstellar medium(ISM),which point toward a change of turbulence properties of the ISM at different scales or novel propagation effects of CRs,and should be properly incorporated in the indirect detection of dark matter via anti-matter particles.