浅析地理国情基础数据采集中的问题

地理国情普查是把握本国国情、国力的一项重大调查.国情基础数据作为地理国情普查的根本,提供了认识和把握国情,评估和增强国力的重要信息.本文主要介绍了地理国情普查内业采集基础数据建库流程,总结了采集过程中应遵循的规则,提出了作业中遇到的情况和处理办法.     

东南沿海地理国情普查影像解译应用分析

影像解译是地理国情普查过程中一项重要的基础性工作,影像解译的结果直接影响作业质量、效率.本文选择东南沿海地区具有典型特征的影像,结合我省正在开展的地理国情普查实践,分别采用目视解译、自动解译和人机交互解译三种方法进行解译,从解译精度、效率、应用条件等方面,对比分析了三种方法的优缺点,结果表明:三种解译方法各具优势和不足,解译结果与影像质量、辅助数据质量、地形复杂程度、地物种类等有密切关系,在实际地理国情普查过程中须综合考虑使用.     

地理国情普查中地表覆盖分类数据典型问题解析

由于地理国情普查是一个全新的、有别于其他测绘项目的新兴项目,在生产过程中难免会出现各种各样的问题。本文结合生产实际,对于地表覆盖分类数据生产过程中出现的一些特征明显、问题集中的错误进行归类解析。     

浅谈高原高寒地区遥感影像判读技巧

以西藏怒江流域高原高寒地区为背景,对利用高分辨率遥感影像进行判读时经常遇到的几方面问题,运用实例分析的方法,给出了解决问题的思路,为以后的工作和类似区域遥感影像的判读提供了参考依据。     

Unraveling Hong Kong Geopark experience with visitor-employed photography method

Geoparks have been established around the world with the major objective of protecting significant geoheritage features and reinforcing geoconservation ideas and support through educating visitors. Understanding visitors' perception of geoheritage can inform educational and conservation endeavors. This study used the visitor-employed photography (VEP) method to unravel visitor perception of geoheritage and associated natural and cultural features in the recently designated Hong Kong Global Geopark of China (HKGP). Participants were asked to take photographs of scenes with an effect on their experience in the HKGP and to elaborate in a logbook the chosen subject, reason of choice, and effect on their travel experience. Aimed at capturing real-time and organic experiences, it was found that geoheritage plays a major role in HKGP visits. Visitors develop strong emotional connections with nature through appreciating and learning about prominent features of both small and landscape scales. However, a mismatch was found between visitor belief or incorrect geological or geomorphological knowledge with inherently strong enthusiasm in deciphering the science behind geoheritage. The findings permit development of a new approach of geopark interpretation, commencing with aesthetic and emotional connections with geoheritage features. Modification of fixed on-site provisions and guiding services directed at visitor interests can better spread geoheritage knowledge and reinforce geoconservation ideas. Modeling after overseas practices, a park ranger system, audio guide devices and smart phone applications are essential to achieve meritorious geopark management, appreciation, and enjoyment.     

基于反射地震资料探讨泥河湾盆地的新生代和中生代地层

查明泥河湾盆地新生界及中生界地层序列及基底的分布与赋存形态是研究泥河湾盆地形成机制的基础性工作。本研究在泥河湾盆地桑干河与壶流河交接处附近采集了四条测线的反射地震数据,通过对精细处理后的地震剖面进行详细分析,在剖面上厘定了三个具有明显强反射标志的地层,即古近系的玄武岩、侏罗系上统的含煤地层和侏罗系下统的含煤地层;其中,新近系沉积层与古近系玄武岩界面在地震剖面上出现的双程旅行时为0.3~0.6s,深度范围为300~500m,而第四系泥河湾组底界由南西到北东逐渐加深,其界面深度为200~300m;侏罗系上统含煤地层在地震剖面上出现的双程旅行时在0.8s上下波动,其深度约为1200m,探测出侏罗系上统顶界面的深度范围为800~1100m;侏罗系下统含煤地层在地震剖面上出现的双程旅行时为1.0~1.4s,深度范围为1800~2000m,由此推测出中生界侏罗系与古生界寒武系地层分界线的深度为2000m左右;根据地震反射波阻抗差别推测出新元古界和太古界地层的分界面在地震剖面上出现的时间约为2.5s,其深度为4000m左右。本研究通过四条反射地震测线的数据基本上查明了泥河湾盆地位于探测区处第四系泥河湾组底界面的深度分布范围及起伏形态、侏罗系上统顶界面和下统底界面的大致埋深,为查明泥河湾盆地新生界及中生界地层序列提供了基础性的参考信息。     

A model of Jupiter's magnetospheric magnetic field with variable magnetopause flaring

We present a new model of the jovian magnetosphere in which the flaring of the magnetopause boundary can be varied. Magnetopause flaring is expected to vary due to changing conditions in the upstream interplanetary medium, related both to the dynamic pressure of the solar wind, and to changes in the direction of the interplanetary magnetic field. The model includes a tilted dipole field, which is screened by the magnetopause, a tail field current system, and the field of a screened equatorial current disc.     

The iron Kα lines as a tool for magnetic field estimations in non-flat accretion flows

Observations of AGNs and microquasars by ASCA, RXTE, Chandra and XMM-Newton indicate the existence of broad X-ray emission lines of ionized heavy elements in their spectra. Such spectral lines were discovered also in X-ray spectra of neutron stars and X-ray afterglows of GRBs. Recently, Zakharov et al. [MNRAS 342 (2003) 1325] described a procedure to estimate an upper limit of the magnetic fields in regions from which X-ray photons are emitted. The authors simulated typical profiles of the iron Kα line in the presence of magnetic field and compared them with observational data in the framework of the widely accepted accretion disk model. Here we further consider typical Zeeman splitting in the framework of a model of non-flat accretion flows, which is a generalization of previous consideration into non-equatorial plane motion of particles emitting X-ray photons. Using perspective facilities of space borne instruments (e.g., Constellation-X mission) a better resolution of the blue peak structure of iron Kα line will allow to evaluate the magnetic fields with higher accuracy.     

Anharmonicity effects in bounce motion of particles

Equations for parallel motion for a particle trapped in a magnetic field have been considered and improved solutions of differential equations have been derived. The expressions for the change in energy of the particle (Δw) and diffusion coefficient (D_ww) have been presented in a simple form using the improved solution.     

Solar wind-magnetosphere interaction as simulated by a 3-D em particle code

We have studied the solar wind-magnetosphere interaction using a 3-D electromagnetic particle code. The results for an unmagnetized solar wind plasma streaming past a dipole magnetic field show the formation of a magnetopause and a magnetotail, the penetration of energetic particles into cusps and radiation belt and dawn-dusk asymmetries. The effects of interplanetary magnetic field (IMF) have been investigated in a similar way as done by MHD simulations. The simulation results with a southward IMF show the shrunk magnetosphere with great particle entry into the cusps and nightside magnetosphere. This is a signature of a magnetic reconnection at the dayside magnetopause. After a quasi-stable state is established with an unmagnetized solar wind we switched on a solar wind with an northward IMF. In this case the significant changes take place in the magnetotail. The waving motion was seen in the magnetotail and its length was shortened. This phenomena are consistent with the reconnections which occur at the high latitude magnetopause. In our simulations kinetic effects will determine the self-consistent anomalous resistivity in the magnetopause that causes reconnections.Deceased January 24, 1993; R. Bunemanet al. 1993.