辽宁省地下水动态成因类型分析

根据辽宁省2006—2010年地下水水位实际监测数据,分析地下水水位动态变化规律、形成原因及发展趋势,再结合地下水动态变化的自然与人为影响控制因素,以及地下水的补给、径流、排泄条件等,将辽宁省地下水动态成因类型划分为:气候型、开采型、灌溉型、水文型和径流型,经过较为全面系统的统计分析计算,绘制出地下水动态变化历时曲线,对五种地下水动态成因类型分别予以较为详细的综合分析研究,总结出辽宁省地下水动态变化规律特征。     

地质雷达在活动断裂研究中的应用

对于快速发生沉积和侵蚀的地区,断裂附近的古地震遗迹会很快被掩埋。获取这些地区断裂的位置、上断点的埋深和标志层的断距等方面的数据至关重要。本文利用地质雷达探测技术探测这些被埋藏的古地震遗迹。以北京平原区正断性质的新夏垫断裂和青藏高原东北缘六盘山地区逆冲性质的六盘山东麓断裂为实验区。通过探测发现,对于断裂两侧地表覆盖层主要为粉土或粉质粘土的新夏垫断裂,地质雷达可精确定位断裂通过的位置,指示上断点的埋深,但无法在地质雷达剖面上识别出各套地层。对于在T1基座阶地上通过的六盘山东麓断裂,地质雷达不但可以精确定位断裂的位置,而且可以在地质雷达剖面上识别出各套地层,进而求得断裂两侧基座的断距。     

AIPS对综合孔径展源的图象处理

本文介绍了用美国国立射电天文台图象处理软件系统—AIPS对综合孔径VLA观测数据的处理方法,特别是对展源,要得到高质量的图象,在编辑及成图中要注意的事项。作者根据自己的实际工作,总结了用AIPS进行图象处理的经验。     

Is TOL 1326-379 a Prototype of γ-Ray Emitting FR0 Radio Galaxy?

With the possible spacial association to the Fermi/LAT source 3FGL J 1330.0-3818,TOL 1326-379 may be the first one that is identified as a γ-ray emitting Fanaro...     

人工观测与自动仪器观测的对比分析

文章利用察右中旗2010年人工观测与自动仪器观测的对比分析,分析两种观测技术获取的气象数据所存在的差异,确保结果的科学性,为自动站业务化运行和气候资料的连续性提供一定参考依据。     

广西右江河谷2008年芒果低温寒害调查分析

通过对广西右江河谷四县(区)2008年低温期间气象要素资料、气候特点进行分析统计,结合芒果的生物学特性、物候发育期及农业气象灾害指标,探讨此次低温寒害天气对右江河谷芒果生产的影响,并提出相应的生产防御对策,以达到趋利避害.     

Incoherent scatter spectrum of ionospheric plasma with an anisotropic temperature ion distribution

The expression of anisotropic temperature ion distribution function under the 13-moment approximation is obtained by solving a set of moment equations based on the Boltzmann equation for a relaxation collision model and with consideration of the anisotropic temperature ion distribution. And the incoherent scatter spectrum with an anisotropic temperature ion distribution is simulated in different directions based on the electromagnetic radiation theory of Sheffield. The effects of different electrical field strengths, ratios of electron temperature to ion temperature, and ion-neutral collision frequencies on the incoherent scatter spectrum are all discussed. Finally, the value of theoretical simulation is compared with the measured value of incoherent scattering spectrum. The result show that the incoherent scatter spectrum of ions seriously deviates from the form of the Maxwellian distribution in the equilibrium state. This phenomenon can be attributed to the effects of anisotropic temperature ion distribution, the larger convection electric field, and other factors in high latitude ionosphere.     

Global-Scale Coupling Characteristics between Geomagnetic Storms and Ionospheric Disturbances

Geomagnetism and Aeronomy - To explore the global-scale coupling characteristics between ionospheric disturbances and geomagnetic storms, and research the near-Earth space environment, the time...     

A complicated solar eruption event on 2003 October 26

We present multi-wavelength observations of a complicated solar eruption event to associate with an X1.2 flare and a Coronal Mass Ejection (CME) on 2003 October 26. The soft X-ray profile shows a possibility for occurrence of two flares with peaks around 06:20 and 07:00 UT. According to our observations, there are many evidences to show that they are corresponding to two energy releases. The first one produces type II, type III, moving type IV continua, a decimetric burst (DCIM) and strong emissions at Hα, 195 and 1600 Å; While the second energy release only produces a group of RS-III bursts, DCIM and Hα emissions. It appears that the first energy release is associated with a CME, while the second CME is quiet. Such observational difference between two energy releases is found indicating two magnetic reconnection processes occurrence with different plasma situation.