Spontaneous superharmonic internal wave excitation by modal interactions in uniform and nonuniform stratifications     

《Dynamics of Atmospheres and Oceans》2020

  相似文献   

X-ray observations of distant Abell clusters     

E. Rizza  J. O. Burns  M. J. Ledlow  F. N. Owen  W. Voges  & M. Bliton 《Monthly notices of the Royal Astronomical Society》1998,301(2):328-342

We present results from a ROSAT HRI study of 11 distant ( z  ∼ 0.2–0.3) Abell clusters. We have performed a morphological analysis to search for and quantify substructure in the clusters. About 70 per cent of the sample shows significant evidence of substructure in the form of centroid shift or obvious X-ray clumps. We examine the clusters for the presence of cooling flows, and determine the physical properties of the ICM by deprojecting the HRI data. Nine of the clusters have central cooling times less than the age of the system, in agreement with fractions determined from nearby, X-ray-bright samples. Additional PSPC results are presented for four clusters in the sample, and ASCA results for six clusters. The temperatures and metallicities for these distant clusters appear to be consistent with nearby clusters of similar richness.  相似文献   

Mass constraints from multiphase cooling flow models     

Peter A. Thomas 《Monthly notices of the Royal Astronomical Society》1998,299(2):349-356

I review the multiphase cooling flow equations that reduce to a relatively simple form for a wide class of self-similar density distributions described by the single parameter, k , first introduced by Nulsen. It is shown that steady-state cooling flows are not consistent with all possible emissivity profiles, which can therefore be used as a test of the theory. In combination, they provide strong constraints on the temperature profile and mass distribution within the cooling radius. The model is applied to ROSAT HRI data for three rich clusters. At one extreme ( K  ∼ 1) these show evidence for cores in the mass distribution of size 110–140 h ⁻¹₅₀ kpc and have temperatures that decline towards the flow centre. At the other ( k ∈ ∞), the mass density and gas temperature both rise sharply towards the flow centre. The former are more consistent with observations which usually show a lower emission-weighted temperature within the cooling flow than from the cluster as a whole. The requirement that the solutions have a temperature gradient that is non-increasing towards the cluster centre limits the matter density gradient to be shallower than ρ_grav ∝∼  r ^−1.2 in the cluster core.  相似文献   

水准椭球的纬向密度分布   总被引：9，自引：1，他引：8  

郝晓光  许厚泽 《测绘学报》1998,27(4):345-351

本文推导了旋转椭球极点重力与赤道重力的密度积分公式。按照１９８０大地参考系统及水准椭球的“极点重力条件”和“赤道重力条件”,从数学上证明了地球的“赤道径向平均密度”大于“极点径向平均密度”,并给出了水准椭球纬向密度分布的估算公式;进而提出了“地球的径向平均密度按纬向正常分布”的假说。  相似文献   

L1估计的分布及统计性质   总被引：3，自引：0，他引：3  

王志忠 《测绘工程》1998,7(2):22-27

推导了Ｌ１估计的密度函数,讨论了Ｌ１估计的统计性质,证明Ｌ１估计是无偏估计,同时还证明Ｌ１估计优于ＬＳ估计。  相似文献   

五大连池近代火山老黑山火烧山火山喷发过程的考察研究   总被引：4，自引：0，他引：4  

任锦章  白志达 《东北地震研究》1998,14(1):76-83

作者在已有工作的基础上,以当代火山学的研究思路和观点,为恢复五大连池两个近代火山,老黑山火烧山的喷发历史过程进行了野外考察研究工作。老黑山火山锥是由三套不同的碎屑堆积物组成。在锥体的南侧、东侧和西侧以及北测和北西侧有５个熔岩溢出口,按它们形成先后关系,认为有早、中、晚三期熔岩流。本文还对老黑山火山锥上的寄生火山、结壳熔岩与渣状熔岩的分布、流动特点及形成的控制因素进行了分析讨论。最后得出结论：老黑山火山是经多期次喷发活动形成的。火烧山火山锥是一碎屑化泡沫化程度很低的浮岩块和熔岩碎块组成,同老黑山有明显区别。  相似文献   

用于便携式γ射线康普顿背散射扫描仪的多道分析器研制     

杜洪  丁厚本 《CT理论与应用研究》1998,7(2):44-48

本文简介了康普顿背散射扫描仪（ＣＢＳ）的基本原理,优点,阐述了便携式ＣＢＳ的特点和对ＣＢＳ多道分析器的要求,介绍了一种多道分析器的指标,电路原理,工作过程和稳峰技术。  相似文献   

The impact of cooling flows on the T_X–L_Bol relation for the most luminous clusters     

S. W. Allen  & A. C. Fabian 《Monthly notices of the Royal Astronomical Society》1998,297(3):L57-L62

We examine the effects of cooling flows on the T _X– L _Bol relation for a sample of the most X-ray luminous ( L _Bol > 10⁴⁵ erg s⁻¹) clusters of galaxies known. Using high-quality ASCA X-ray spectra and ROSAT images we explicitly account for the effects of cooling flows on the X-ray properties of the clusters and show that this reduces the previously noted dispersion in the T _X– L _Bol relationship. More importantly, the slope of the relationship is flattened from L _Bol ∝  T ³_X to approximately L _Bol ∝  T ²_X, in agreement with recent theoretical models which include the effects of shocks and pre-heating on the X-ray gas. We find no evidence for evolution in the T _X– L _Bol relation within z  ∼ 0.3. Our results demonstrate that the effects of cooling flows must be accounted for before cosmological parameters can be determined from X-ray observations of clusters. The results presented here should provide a reliable basis for modelling the T _X– L _Bol relation at high X-ray luminosities.  相似文献   

The relationship between cooling flows and metallicity measurements for X-ray-luminous clusters     

S. W. Allen  & A. C. Fabian 《Monthly notices of the Royal Astronomical Society》1998,297(3):L63-L68

We explore the relationship between the metallicity of the intracluster gas in clusters of galaxies, determined by X-ray spectroscopy, and the presence of cooling flows. Using ASCA spectra and ROSAT images, we demonstrate a clear segregation between the metallicities of clusters with and without cooling flows. On average, cooling-flow clusters have an emission-weighted metallicity a factor ∼ 1.8 times higher than that of non-cooling-flow systems. We suggest that this is caused by the presence of metallicity gradients in the cooling-flow clusters, coupled with the sharply peaked X-ray surface brightness profiles of these systems. Non-cooling-flow clusters have much flatter X-ray surface brightness distributions and are thought to have undergone recent merger events, which may have mixed the central high-metallicity gas with the surrounding less metal-rich material. We find no evidence for evolution in the emission-weighted metallicities of clusters within z  ∼ 0.3.  相似文献   

Role of barotropic,baroclinic and combined barotropic-baroclinic instability for the growth of monsoon depressions and mid-tropospheric cyclones     

B. N. Goswami  R. N. Keshavamurty  V. Satyan 《Journal of Earth System Science》1980,89(1):79-97

A detailed barotropic, baroclinic and combined barotropic-baroclinic stability analysis has been carried out with mean monsoon zonal currents over western India, eastern India and S.E. Asia. The lower and middle tropospheric zonal wind profiles over western India are barotropically unstable. The structure and growth rate of these modes agree well with the observed features of the midtropospheric cyclones. Similar profiles over eastern India and S.E. Asia, however, are barotropically stable. This is attributed to weak horizontal shear, inherent to these profiles. The upper tropospheric profiles, on the other hand, are barotropically unstable throughout the whole region. The features of these unstable modes agree with those of observed easterly waves. The baroclinic and combined barotropic-baroclinic stability analyses show that the baroclinic effects are not important in tropics. Though the barotropic instability of the mean zonal current seems to be res ponsible for the initial growth of the mid-tropospheric cyclones, neither barotropic nor baroclinic instability of the mean zonal current seem to explain the observed features of the monsoon depressions.  相似文献