IAP GCM模式大气波谱结构及其在厄尔尼诺年的异常     

王盘兴  刘家铭  沈素红 《南京气象学院学报》1992,(1)

本文分析了中国科学院大气物理研究所大气环流模式(IAP GCM)模式大气波谱结构(沿纬圈的谐波波谱和时域上的频率谱)及其在厄尔尼诺年的异常。结果表明,超长波是低纬波动的主要空间形式,准40天振荡在一定地理区域内显著存在,并与观测结果有一定联系,它们在厄尔尼诺年均发生明显异常。本工作对鉴定GCM性能及开发GCM的研究领域可能是一种有益的尝试。  相似文献   

Multi-spacecraft observations of heliographic structure of the solar wind speed     

W. Miyake

K. Kobayashi

K. -I. Oyama  T. Mukai

T. Abe

T. Terasawa

K. Yumoto  T. Saito

K. Hirao

A. J. Lazarus

A. D. Johnstone 《Planetary and Space Science》1988,36(12):1329-1342

Multi-spacecraft observations in the interplanetary space are used to build up a picture of the distribution of solar wind velocities in heliographic latitude and longitude. Analyses are made for the solar wind data obtained by Sakigake, Suisei, IMP-8 and Giotto between late 1985 and early 1987. Until Janaury 1986, high-speed streams were extended across the equator from the high latitudes of the heliosphere. After March 1986, high-speed streams were rarely seen on the equator. Although there remained a slight wavy pattern in latitude-longitude structure, low-speed streams were basically ranged along the equator. After January 1987, the amplitude of this wavy pattern was further diminished and low-speed regions were completely aligned to the equator.  相似文献   

研究Lienard方程闭轨线的一种方法     

胡军胜 《广东海洋大学学报》2000,20(2):56-58

结合实例分析说明 Filippov变换在研究 Lienard方程不存在闭轨线时的运用方法  相似文献   

锂矿盐湖锂分离提取新方法研究取得阶段性成果   总被引：1，自引：0，他引：1       下载免费PDF全文

宋粤华 《盐湖研究》2000,8(2):77-78

锂矿盐湖锂分离提取新方法研究”是中国科学院“西部之光”计划资助的项目,由中国科学院青海盐湖研究所青年科研小组承担并完成。该项目主要针对青海丰富的盐湖资源,以最典型和最具代表性的锂矿盐湖———东台吉乃尔盐湖为研究对象,开展盐湖卤水提锂新方法的研究。锂及其盐类是国民经济和国防建设中具有重要意义的战略物资,也是与人们生活息息相关的能源材料。近10年来,锂的国际消费量以每年6%—7%的速度增长。国内锂盐的消费市场主要在高能电池业、炼铝工业、制冷剂、制药、化学试剂和润滑剂等,近年来需求量一直呈上升趋势。锂的矿产有两大…  相似文献   

我国卤水溴资源及其开发前景展望   总被引：5，自引：0，他引：5       下载免费PDF全文

乌志明  温现明 《盐湖研究》2000,8(2):59-67

溴在自然界无独立的矿物 ,呈强分散性稀有元素 ,散布在地壳水圈里 ,以油气田地下卤水、盐湖卤水、矿场盐卤水含溴浓度相对较高。溴在国民经济的用途广泛 ,是我国紧缺物资 ,产不敷消。而我国卤水溴资源分布广泛 ,类型齐全 ,同时常伴有K、B、I、Li等多种有用组分。充分发挥各类卤水溴资源特点 ,提高卤水溴资源综合利用水平 ,其开发前景广阔  相似文献   

同仁双朋西金矿浮选尾矿中提铜扩大试验的研究          下载免费PDF全文

龙光明  康永峰 《盐湖研究》2000,8(2):22-28

在小试的工艺基础上 ,对双朋西金矿浮选后的尾矿进行铜、金回收扩大试验。对铜的浸取试验结果表明 ,本工艺对该尾矿具有较高的铜浸取率和回收率  相似文献   

The ionospheric effects in D-layer and solar proton precipitation zones during the 16 February 1984 event     

M. I. Beloglazov  G. P. Beloglazova  E. V. Vashenyuk  G. A. Petrova  O. I. Shumilov  V. A. Shishaev

I. N. Zabavina

V. I. Nesterov 《Planetary and Space Science》1990,38(12):1479-1486

The results of the geophysical and VLF (10–16 kHz) radio propagation measurements on the net of observatories during the solar proton event on 16 February 1984 are analysed. It is shown that the abnormal ionization region caused by solar protons consisted of two parts. One of them was the direct access zone in the middle and morning side of the polar cap, the other was the precipitation region of the quasi-trapped particles in the mid-day and evening sectors of the auroral zone. The probable profiles of the lower ionosphere electron density are determined from the VLF and satellite data of the energetic spectra at the maximum penetration. It is shown that the effective electron concentration at the height 45 km was close to 10³ cm⁻³.  相似文献   

Secular tidal changes in lunar orbit and Earth rotation     

James?G.?WilliamsEmail authorView author&#;s OrcID profile  Dale?H.?Boggs 《Celestial Mechanics and Dynamical Astronomy》2016,126(1-3):89-129

Small tidal forces in the Earth–Moon system cause detectable changes in the orbit. Tidal energy dissipation causes secular rates in the lunar mean motion n, semimajor axis a, and eccentricity e. Terrestrial dissipation causes most of the tidal change in n and a, but lunar dissipation decreases eccentricity rate. Terrestrial tidal dissipation also slows the rotation of the Earth and increases obliquity. A tidal acceleration model is used for integration of the lunar orbit. Analysis of lunar laser ranging (LLR) data provides two or three terrestrial and two lunar dissipation parameters. Additional parameters come from geophysical knowledge of terrestrial tides. When those parameters are converted to secular rates for orbit elements, one obtains dn/dt = \(-25.97\pm 0.05 ''/\)cent\(^{2}\), da/dt = 38.30 ± 0.08 mm/year, and di/dt = ?0.5 ± 0.1 \(\upmu \)as/year. Solving for two terrestrial time delays and an extra de/dt from unspecified causes gives \(\sim \) \(3\times 10^{-12}\)/year for the latter; solving for three LLR tidal time delays without the extra de/dt gives a larger phase lag of the N2 tide so that total de/dt = \((1.50 \pm 0.10)\times 10^{-11}\)/year. For total dn/dt, there is \(\le \)1 % difference between geophysical models of average tidal dissipation in oceans and solid Earth and LLR results, and most of that difference comes from diurnal tides. The geophysical model predicts that tidal deceleration of Earth rotation is \(-1316 ''\)/cent\(^{2}\) or 87.5 s/cent\(^{2}\) for UT1-AT, a 2.395 ms/cent increase in the length of day, and an obliquity rate of 9 \(\upmu \)as/year. For evolution during past times of slow recession, the eccentricity rate can be negative.  相似文献   

Line-of-Sight Anisotropies in the Cosmic Dawn and Epoch of Reionization 21-cm Power Spectrum     

Suman?MajumdarEmail authorView author&#;s OrcID profile  Kanan?K.?Datta  Raghunath?Ghara  Rajesh?Mondal  T.?Roy?Choudhury  Somnath?Bharadwaj  Sk.?Saiyad?Ali  Abhirup?Datta 《Journal of Astrophysics and Astronomy》2016,37(4):32

The line-of-sight direction in the redshifted 21-cm signal coming from the cosmic dawn and the epoch of reionization is quite unique in many ways compared to any other cosmological signal. Different unique effects, such as the evolution history of the signal, non-linear peculiar velocities of the matter etc. will imprint their signature along the line-of-sight axis of the observed signal. One of the major goals of the future SKA-LOW radio interferometer is to observe the cosmic dawn and the epoch of reionization through this 21-cm signal. It is thus important to understand how these various effects affect the signal for its actual detection and proper interpretation. For more than one and half decades, various groups in India have been actively trying to understand and quantify the different line-of-sight effects that are present in this signal through analytical models and simulations. In many ways the importance of this sub-field under 21-cm cosmology have been identified, highlighted and pushed forward by the Indian community. In this article, we briefly describe their contribution and implication of these effects in the context of the future surveys of the cosmic dawn and the epoch of reionization that will be conducted by the SKA-LOW.  相似文献   

Characteristics of convection and overshooting in RGB and AGB stars     

Xiang-Jun Lai    Yan Li  National Astronomical Observatories/ Yunnan Observatory  Chinese Academy of Sciences  Kunming  China  Key Laboratory for the Structure  Evolution of Celestial Objects  China Graduate University of Chinese Academy of Sciences  Beijing  China. 《中国天文和天体物理学报》2011,(10)

Based on the turbulent convection model (TCM) of Li & Yang, we have studied the characteristics of turbulent convection in the envelopes of 2 and 5M⊙ stars at the red giant branch and asymptotic giant branch phases. The TCM has been successfully applied over the entire convective envelopes, including the convective unstable zone and the overshooting regions. We find that the convective motions become progressively stronger when the stellar models are located farther up along the Hayashi line. In the convect...  相似文献