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101.
The short-term evolution of spheroidal galaxies has been explored by S. Chandrasekhar et al. and G. S. Sunder et al. In this paper, we study their long-term evolution with Laskar's method of frequency analysis. The main new results are as follows: (1) There exists a unique equilibrium, which is spherically symmetric. This equilibrium has a critical linear stability. (2) Generally speaking, the semi-axes exhibit quasiperiodic or nearly quasi-periodic (in a time scale longer than a Hubble time) oscillations around the radius of the above-mentioned equilibrium, so the equilibrium is practically stable. (3) There are cases in which one of the semi-axes tends fast to zero while the other to some finite value. The limit state is generally planar rather than linear, i.e. it is the symmetric semi-axis that tends to zero. This implies that some disk galaxies may have originated from spheroidal pregalaxy material. 相似文献
102.
湖北省降水量的周期分析 总被引:8,自引:0,他引:8
结合降水量对农业生产的影响特点将全年降水量分成5个阶段,根据聚类分析的结果将不同的时段的降水量进行分区,由此对全省的降水量做自相关分析和功率谱分析,从而发现了降水量的变化周期。 相似文献
103.
Glenn E. Shaw 《Pure and Applied Geophysics》1980,119(2):231-247
Layers of stratospheric aerosol with optical thicknesses as small as 10–4 cause noticeable perturbations in the monochromatic logarithmic brightness gradient,G, and the color ratio,C, of the twilight sky. Modeling of the twilight's radiant properties shows that definite single-valued relationships exist between maxima inC or minima inG and optical thickness, , physical thickness h, and mean altitude,
, of stratospheric layers. It is therefore possible to determine , h and
and monitor their variations by performing either single wavelength measurements ofG or two-wavelength spectrophotometric measurements ofC. The presence of haze in the lower troposphere and the occurrence of multiple scattering both have relatively minor influences on the recovery of the stratospheric dust properties, provided that 10<
<30 km.Formal mathematical inversions of the single-scattering twilight equations are possible in principle, but difficult in practice because of non-linearities. Inversions incorporating an iterative linearization process with constrained smoothing, successfully recovered the features of the haze layer, but tended to oversmooth the vertical profile and underestimate the mean altitude of the haze layer. 相似文献
104.
J. Röttger 《Pure and Applied Geophysics》1980,118(1):494-527
Powerful VHF radars are capable of almost continuously monitoring the threedimensional velocity vector and the distribution of turbulence in the middle atmosphere, i.e. the stratosphere and mesosphere. Methods of radar investigations of the middle atmosphere are outlined and the basic parameters, mean and fluctuating velocities as well as reflectivity and persistency of atmospheric structures, are defined. Results of radar investigations are described which show that the tropopause level as well as a criterion on the stability of the lower stratosphere can be deduced. Besides mean wind velocities, VHF radars can measure instantaneous velocities due to acoustic gravity waves. The interaction of gravity waves with the background wind is discussed, and it is shown that cumulus convection is an effective source of gravity waves in the lower stratosphere. The vertical microstructure of the stratosphere, manifesting itself in thin stratified sheets in which temperature steps occur, is investigated by applying knowledge from investigations of the oceanic thermocline. Possible origins, like shear generation and lateral convection of the microstructure of the stratosphere, are discussed. Observations of gravity waves in the mesosphere are reviewed and their connection with turbulence structures is pointed out. Finally, some open questions which could be answered by further VHF radar investigations are summarized. 相似文献
105.
Height distribution of the stratospheric aerosol extinction coefficient was measured in the altitude range 10 to 20 km by a balloon-borne multi-color sunphotometer in May 1978. It is demonstrated that detailed structures of the distribution of stratospheric aerosol can be remotely measured by the solar occultation method as well as by lidar andin situ particle counter observations. In the aerosol layer appearing at 18 km altitude the extinction coefficient at 800–1000 nm wavelength reached to 3×10–7 m–1, which was reasonable compared with lidar observations. Wavelength dependence of the aerosol optical depth was crudely estimated to be proportional to
–1.5. 相似文献
106.
Li Chongyin 《大气科学进展》1998,15(1):31-40
The data analyses found at first that the air—sea system in the northwestern Pacific region has clear systematical quasi—decadal
oscillation, such as the surface air temperature, the subtropical high activities over the northwestern Pacific and the SSTA
which has different time-scale features from the temporal variation with 3–4 years period of SSTA in the equatorial Pacific.
In East Asia, the climate variations, such as the surface air temperature, the precipitation and the beginning date of Mei-yu
in the Yangtze River basin, also have clear quasi-decadal oscillation. They can be regarded as the influences of quasi-decadal
oscillation of air-sea system in the northwestern Pacific region.
This research was supported by the Chinese Academy of Sciences and ‘95’ National Project- “Short-Range Climate Production
System”. 相似文献
107.
异常东亚冬季风激发ENSO的数值模拟研究 总被引:40,自引:11,他引:29
利用中国科学院大气物理研究所发展的热带太平洋环流模式(OGCM)和海-气耦合模式(CGCM)分别就冬半年东亚冬季风异常对赤道太平洋的作用进行了数值模拟研究。结果清楚地表明,无论在 OGCM 中还是在 CGCM 中,持续的冬季风强异常将引起赤道中东太平洋海表水温(SST)的明显正异常,其分布类似观测到的El Ni?o事件;而持续的冬季风弱异常将引起赤道中东太平洋SST的明显负异常,其分布十分类似观测到的La Ni?a事件。因此,数值模拟进一步证实了我们过去从资料诊断和理论分析中得到的结论,即东亚冬季风异常是激发产生 ENSO 的重要机制。对模式资料的分析还清楚表明,异常东亚冬季风将激发异常海洋Kelvin波和使热带大气季节内振荡出现强异常,它们是激发ENSO的重要物理因素,这与观测资料的分析结果相一致。 相似文献
108.
����ˮϵͳ��������ѧ�о� 总被引:1,自引:1,他引:0
?????????????????????????????????е???????,???????????????????????????????????????????????????????????????HLS??????????????????? 相似文献
109.
利用双阳台水管观测资料检测地球自由振荡 总被引:2,自引:2,他引:0
基于双阳台水管倾斜仪的数字化观测资料,利用功率谱密度估计方法,在没有对资料进行去固体潮处理的情况下,准确获得了2004年12月26日苏门答腊大地震激发的0S3~0S31基频球型自由振荡。并与PREM模型的理论自由振荡周期进行了对比,发现实测振荡周期与PREM预测的振荡周期相吻合,除0S3、0S4振型的观测周期和PREM模型理论周期的相对误差大于0.3%外,其他振型的观测周期和PREM模型理论周期的相对误差大都集中在0.1%左右。同时还检测到了5个谐频球型振荡和8个环型振荡。 相似文献
110.
������������ģ�ļ��� 总被引:1,自引:0,他引:1
??????????????????(Runge??Kutta)????????PREM??????????????????λ??????????????????????????????200 s??????????????????ε??????????????????????????????????仯???????????????о??????λ???????е?仯?????????????:??????????????????????????????仯?????, 20???????????????μ????????????Dziewonski??Anderson??????, ?????????????0.25%????? 相似文献