湖大井动水位观测及其分析

本文对湖大水井的动水位观测作了介绍。根据观测资料,对动水位与流量、动水位与气压的关系以及水振波的控震能力等作了初步分析。     

地下水"恒流式"单井综合观测方法

以探索水位与水化学单井综合观测新方法为目的，建立了改性动水位概念，即恒定小流量状态下的井孔动水位。理论分析和实验表明，改性动水位与同一井孔对应的静水位之间相差一恒定水位落差。根据这一结果，可将观测得到的改性动水位值订正成相对应的静水位值。由此建立了以改性动水位和传统水化学为观测对象的“恒流式”单井综合观测方法，从而实现了静水位与传统水化学的单井综合观测。     

鲁23井“动水位”观测的分析

本文介绍了鲁23井“动水位”观测情况。提出了一个分析有泄流的“动水位”的新方法,即把流量换算成水位,以等效静水位来表示“动水位”与流量。由于把“动水位”与流量用一个量来计算,从而为“动水位”观测定量的、统一的分析研究提供了新的方法。这对提高“动水位”井的监测预报地震能力起一定的作用。 本文还以鲁23井“动水位”观测资料为例,利用新方法进行处理的观测分析结果与理论研究结果是一致的。     

泄流量对动水位观测影响的分析

利用深井动水位观测资料预报地震,已经被国内外地震学家进行深入研究,并得到了许多珍贵的震例资料。从多年的观测实践认识到,观测装置系统对动水位记录地震信息量是关键环节,泄流量的调节也是提高动水位观测质量的重要因素。     

浮子数字水位仪动水位观测实验

针对投入式水位仪存在稳定性差、零漂大等缺点,研制浮子式JS-1数字水位仪,基于观测原理和仪器结构,在苏18井开展动水位观测实验,结果发现:JS-1数字水位仪在动水位观测中可行,产出数据质量优良,并且在对零漂控制、观测数据质量、观测精度等方面具有一定优势。     

综合动水位与流量值的等效静水位及其计算方法探索

中国地震地下流体观测网动水位观测中,一般同时观测水位与泄流量2个测项,产生2类动态,分别进行处理与分析。对含水层应力状态变化的信息,有时得到2种相反的结果。针对这种不合理的现状,以流体动力学理论为基础,探索了动水位观测井中水位与流量的关系,提出了等效静水位的概念,把水位与流量2个观测量合成为1个统一的物理量,建立了相应的计算方法,并用东水3井与聊古1井的观测资料进行了检验     

汶川地震前后水位频谱特征分析

以频谱分析方法作为理论基础,采用周期图法计算汶川地震前后距震中500 km以内10口观测井水位（包括动水位与静水位）的功率谱,对比分析2009年无大震年份同时期的数据,研究结果表明：水位的频域特征受制于观测井的地质构造背景、观测方式和观测深度;水位的波动能量主要集中于大于4天与小于0.5天周期,震后水位波动能量则集中在大于8天的周期;动水位频谱更加丰富.另外,不同井水位的频域响应特征与该井观测层岩性有关,需进一步研究.     

唐山矿井模拟与数字水位的记震能力对比分析

介绍了唐山矿井模拟水位与数字水位观测的基本情况,对2004年7月至12月11次全球7级以上地震引起唐山矿井模拟水位与数字水位水震波特征进行了对比分析。结果表明数字水位有较模拟水位的记震特征易识别,水震波初动清楚,资料连续,误差小等优点,但数字水位采样率低,水震波记录存在畸变。     

“动水位”异常特征与敏感原因分析

我国地震地下水动态观测井网建立以来所取得的资料表明,同样是承压水,静水位和动水位的映震能力有明显不同,论文通过大量实例及统计结果说明,动水位的映震能力明显优于静水位,并从理论上探讨了“动水位”映震能力强的原因。     

动水位变化与地震短临预报——介绍河间马17号井映震“敏感点”

我国早于1979年开始建设“第二代”深井地下水观测网以来,就已注意到观测动水位(实质是流量)的前兆变化较之静水位更为明显,并强调对地震“敏感点”的观测研究。本文介绍的河北省河间县马17号井就是这类映震“敏感点”的典型实例。该井自1981年投入观测以来,其动水位变化对周围发生的10余次5级以上地震前都有明显的前兆反映,尤其是1985年11月30日邢台任县5.3级地震前据此作出了较好的短临预报。实践表明,马17号井是反映区域应力场的“敏感点”。深入探讨其映震敏感的机理,寻找并监视多个敏感点的动水位、水氡、水溶气体及深部离子成份的变化动态,可能不失为突破中强地震预报难点的一条有效途径。     

OH(6–2) spectra and rotational temperature measurements at Davis, Antarctica

The OH(6 – 2) band was monitored during 1990 at Davis, Antarctica (68.6°S, 78.0°E) using a Czerny-Turner scanning spectrometer. Spectra obtained with a 0.15-nm bandwidth and wavelength steps of 0.005 nm have been recorded in an attempt to isolate auroral features. This has enabled detailed study of weak features in the region 837.5–855.5nm. These weak features can contribute to the apparent intensity of P-branch lines and to the background. Their presence is allowed for in our calculation of rotational temperature, but the P₁ (3) line is excluded because of significant contamination. An average temperature of 221 ± 2K is obtained from a selected data set of 104 spectra. The mid-winter average temperature, for the months of May, June and July, is 224 ± 2K, which is consistent with the 1986 CIRA model values for mid-winter at this height and latitude, but this result is dependent on the choice of transition probabilities. Preliminary assessments of seasonal and diurnal variations in rotational temperature and intensity are presented.     

Lower thermospheric nitric oxide concentrations derived from WINDII observations of the green nightglow continuum at 553.1 nm

Vertical profiles of nitric oxide in the altitude range 90 to 105 km are derived from 553 nm nightglow continuum measurements made with the Wind Imaging Interferometer (WINDII) on the Upper Atmosphere Research Satellite (UARS). The profiles are derived under the assumption that the continuum emission is due entirely to the NO+O air afterglow reaction. Vertical profiles of the atomic oxygen density, which are required to determine the nitric oxide concentrations, are derived from coordinated WINDII measurements of the atomic oxygen OI 557.7 nm nightglow emission. Data coverage for local solar times ranging from 20 h to 04 h, and latitudes ranging from 42°S to 42°N, is achieved by zonally averaging and binning data obtained on 18 nights during a two-month period extending from mid-November 1992 until mid-January 1993. The derived nitric oxide concentrations are significantly smaller than those obtained from rocket measurements of the airglow continuum but they do compare well with model expectations and nitric oxide densities measured using the resonance fluorescence technique on the Solar Mesosphere Explorer satellite. The near-global coverage of the WINDII observations and the similarities to the nitric oxide global morphology established from other satellite measurements strongly suggests that the NO+O reaction is the major source of the continuum near 553 nm and that there is no compelling reason to invoke additional sources of continuum emission in this immediate spectral region.     

火星环境探测结果分析

本文对空间飞行器所观测取得的火星环境的资料进行了分析研究，并对有关火星磁层和电离层及其与太阳风机相互作用的研究结果进行了概述。     

The ALOMAR Rayleigh/Mie/Raman lidar: objectives, configuration, and performance

We report on the development and current capabilities of the ALOMAR Rayleigh/Mie/Raman lidar. This instrument is one of the core instruments of the international ALOMAR facility, located near Andenes in Norway at 69°N and 16°E. The major task of the instrument is to perform advanced studies of the Arctic middle atmosphere over altitudes between about 15 to 90 km on a climatological basis. These studies address questions about the thermal structure of the Arctic middle atmosphere, the dynamical processes acting therein, and of aerosols in the form of stratospheric background aerosol, polar stratospheric clouds, noctilucent clouds, and injected aerosols of volcanic or anthropogenic origin. Furthermore, the lidar is meant to work together with other remote sensing instruments, both ground- and satellite-based, and with balloon- and rocket-borne instruments performing in situ observations. The instrument is basically a twin lidar, using two independent power lasers and two tiltable receiving telescopes. The power lasers are Nd:YAG lasers emitting at wavelengths 1064, 532, and 355 nm and producing 30 pulses per second each. The power lasers are highly stabilized in both their wavelengths and the directions of their laser beams. The laser beams are emitted into the atmosphere fully coaxial with the line-of-sight of the receiving telescopes. The latter use primary mirrors of 1.8 m diameter and are tiltable within 30° off zenith. Their fields-of-view have 180 rad angular diameter. Spectral separation, filtering, and detection of the received photons are made on an optical bench which carries, among a multitude of other optical components, three double Fabry-Perot interferometers (two for 532 and one for 355 nm) and one single Fabry-Perot interferometer (for 1064 nm). A number of separate detector channels also allow registration of photons which are produced by rotational-vibrational and rotational Raman scatter on N₂ and N₂+O₂ molecules, respectively. Currently, up to 36 detector channels simultaneously record the photons collected by the telescopes. The internal and external instrument operations are automated so that this very complex instrument can be operated by a single engineer. Currently the lidar is heavily used for measurements of temperature profiles, of cloud particle properties such as their altitude, particle densities and size distributions, and of stratospheric winds. Due to its very effective spectral and spatial filtering, the lidar has unique capabilities to work in full sunlight. Under these conditions it can measure temperatures up to 65 km altitude and determine particle size distributions of overhead noctilucent clouds. Due to its very high mechanical and optical stability, it can also employed efficiently under marginal weather conditions when data on the middle atmosphere can be collected only through small breaks in the tropospheric cloud layers.     

Stratospheric background aerosol and polar cloud observations by laser backscattersonde within the framework of the European project “Stratospheric Regular Sounding”

The Stratospheric Regular Sounding project was planned to measure regularly the vertical profiles of several tracers like ozone, water vapor, NO_x, ClO_x and BrO_x radicals, aerosol, pressure and temperature, at three latitudes, to discriminate between the transport and photochemical terms which control their distribution. As part of this project, the “Istituto di Fisica dell’Atmosfera” launched nine laser backscattersondes (LABS) on board stratospheric balloons to make observations of background aerosol and PSCs. LABS was launched with an optical particle counter operated by the University of Wyoming. Observations have been performed in the arctic, mid-latitudes and tropical regions in different seasons. Polar stratospheric clouds have been observed in areas inside and outside the polar vortex edge. A background aerosol was observed both in mid-latitudes and in arctic regions with a backscattering ratio of 1.2 at 692 nm. Very stratified aerosol layers, possibly transported into the lower stratosphere by deep convective systems, have been observed in the lower stratosphere between 20 and 29 km in the tropics in the Southern Hemisphere.     

技术职称改革实践中的问题及若干建议

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Hydroxyl (6/2) airglow emission intensity ratios for rotational temperature determination

OH(6/2) Q1/P1 and R₁/P₁ airglow emission intensity ratios, for rotational states up to j = 4.5, are measured to be lower than implied by transition probabilities published by various authors including Mies, Langhoff et al. and Turnbull and Lowe. Experimentally determined relative values of j transitions yield OH(6/2) rotational temperatures 2 K lower than Langhoff et al., 7 K lower than Mies and 13 K lower than Turnbull and Lowe.     

新形势下地震监测预报发展的思考

本文从我国30多年地震监测预报历程、今后监测预报的发展方向以及改进监测预报管理工作等方面简明扼要地阐明了在新形式下如何推进地震监测预报发展的思考,文中所讨论的问题及新思维、新观点,相信对广大读者会带来更多的启迪,以此促进防震减灾事业的不断发展。     

Progress in Earthquake Science and Technology in China: Review and Prospects (Ⅰ)

In the article the author looks back the hard development course and great progress in earth quake science and technology in China during the last near a half of century and expounds the following 3 aspects: (1) The strong desire of the whole society to mitigate seismic disasters and reduce the effect of earthquakes on social-economic live is a great driving force to push forward the development of earthquake science and technology in China; (2) To better ensure people‘ s life and property, sustainable economic development, and social stability is an essential purpose to drive the development of earthquake science and technology in China; and (3) To insist on the dialectical connection of setup of technical system for seismic monitoring with the scientific research of earthquakes and to better handle the relation between crucial task, current scientif ic level, and the feasibility are the important principles to advance the earthquake science and technology in China. Some success and many setbacks in earthquake disaster mitigation consistently enrich our knowledge regarding the complexity of the conditions for earthquake occurrence and the process of earthquake preparation, promote the reconstruction and modernization of technical system for earthquake monitoring, and deepen the scientific research of earthquakes. During the last 5 years, the improvement and modernization of technical system for earthquake monitoring have clearly provided the technical support to study and practice of earthquake prediction and pre caution, give prominence to key problems and broaden the field of scientific research of earth quakes. These have enabled us to get some new recognition of the conditions for earthquake oc currence and process of earthquake preparation, characteristics of seismic disaster, and mecha nism for earthquake generation in China‘s continent. The progress we have made not only en courages us to enhance the effectiveness of earthquake disaster mitigation, but also provides a basis for accelerating further development of earthquake science and technology in China in the new century, especially in the 10th five-year plan. Based on the history reviewed, the author sets forth a general requirement for develop ment of earthquake science and technology in China and brings out 10 aspects to be stressed and strengthened at present and in the future. These are: upgrade and setup of the network of digitized seismic observation; upgrade and setup of the network for observation of seismic pre cursors; setup of the network for observation of strong motion; setup of the laboratories for ex periment on seismic regime; establishment of technical system for seismic information, emer gency command and urgent rescue; research on short-term and imminent earthquake predic tion; research on intermediate- and long-term earthquake prediction; research on attenuation of seismic ground motion, mechanism for seismic disaster, and control on seismic disaster; ba sic research fields related to seismology and geoscience. We expect that these efforts will signifi cantly elevate the level of earthquake science and technology in China to the advanced interna tional level, improve theories, techniques, and methods for earthquake precaution and predic tion, and enhance the effectiveness of earthquake disaster mitigation.