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1.
用国际地球自转服务提供的高精度日长序列△LOD(IERS(EOP99CO4)，和由美国国家环境预报中心(NCEP)对过去的气象资料进行重新分析和计算，提供的轴向大气角动量序列(AAM)来研究大气和带谐潮汐对地球自转变化(△LOD)中高频振荡激发的贡献。由Multitaper功率谱分析表明，△LOD序列在9．13d(天)、13．63d、13．66d、27．55d周期时呈现出比较强的谱峰，这些谱都在95％的显著性水平以上，有比较强的信噪比。从△LOD和AAM之差值序列谱分析结果及地球带谐响应系数k的估计，表明大气不是△LOD的高频变化的主要激发源。根据理论潮汐周期可知，有可能存在其它的激发源，如海洋对地球自转变化的激发。这还有待于进一步深入探讨。 相似文献
2.
大气角动量资料源的变化对研究日长变化激发的贡献 总被引：4，自引：0，他引：4
本文采用1979—1995年间由空间大地测量技术观测和归算的日长变化（△LOD）序列,以及由美国国家气象中心（NMC）和美国国家环境预测中心与美国国家大气研究中心（NCEP／NCAR）利用全球气象资料各自归算的大气角动量（AAM）序列,重新分析、研究和估计了大气对△LOD的激发作用,比较了上述各个大气角动量序列对△LOD激发贡献,得到的主要结果如下：1．NCEP／NCAR用同化后的全球气象资料重新归算的AAM序列比原来NMC的序列具有系统均匀化、噪声小和分辨率高的特点,以及和日长变化的符合度更好．2．采用NCEP／NCAR重新归算的AAM来研究大气在从亚季节性到年际时间尺度上对非潮汐△LOD的激发贡献,得到进一步改善的结果,尤其是在准两年时间尺度上．但是大气仍不能解释全部△LOD化,可能存在其它激发源．3．大气对△LOD高频潮汐项的估计值影响较小,并从△LOD中解算出周年和半年潮汐参数估计的初步结果． 相似文献
3.
大气对地球自转参数（ERP）的高频激发 总被引：4，自引：0，他引：4
本文采用１９８３—１９９２年期间由空间大地测量技术观测和归算的地球自转参数（ＥＲＰ）序列，以及由全球气象资料归算的大气角动量（ＡＡＭ）序列，分析和研究了大气对地球自转参数的日长变化（ＬＯＤ）和极移（ｘ和ｙ）在一个月时间尺度以内的高频激发作用，得到的主要结果如下：１大气对ＬＯＤ分量高频潮汐的估计值存在着影响，但是，潮汐形变参数ｋ／ｃ随时间和频率的变化却是受非大气因素的扰动引起的．２．大气可以解释３０天以下ＬＯＤ非潮汐的大部分变化．３．极移分量３０天以内的高频变化也主要由大气激发．ｘ分量与大气的相关性要强于ｙ分量，而且更为稳定，主要表现为平均时间尺度约为２７天的波动，大气对这个波动的贡献可达７０％． 相似文献
4.
采用从1988－1999年的现代技术测定的高精度极移序列EOP（IERS97C04）推导出激发函数χ^m）和美国国家环境预测中心和美国国家大气研究中心（CNEP／NCAR）提供的大气角动量激发函数χp和χib^p，使用几种数据分析方法，分析了大气对极移高频振荡（12－42cpy)激发贡献，复数小波变换和功率谱分析表明，χ^m和χ^p序列在高频段内呈现比较强的谱峰，它们具有相似的谱特征，比较而言，χib^p在这个频率段内比χ^p要弱些，χ^m和χ^p之间的相关系数分别为0．75（逆向）和0．6（顺向），两个序列之间的平方相关谱的估计值分别在0．5－0．9之间（负频）和0．4－0．6（正频），相位谱表明χ^p(AAM)超前x^m一天左右，这些大气是极移高频变化的主要激发源，特别是在逆向运动上具有更大的贡献，由于它们之间位相差和振幅变化的不稳定性，说明可能存在AAM以外的其他激发源，这个问题有待进一步深入研究。χ 相似文献
5.
大气角动量(AAM) 变化和地球自转变化密切相关,它们可应用于全球环流模型的检验.根据日本气象厅全球环流模型的输出数据计算出AAM 函数,将AAM 函数的模拟值与它的观测值以及地球自转变化序列相比较,来检验该模型对大气角动量的模拟.限于篇幅,仅给出AAM 函数的季节性分量模拟的结果.对于半年项,轴向AAM 函数的气压项和风项的模拟值都偏高,赤道向AAM 函数的气压项和风项很小,因而未予考虑;对于周年项,轴向AAM函数气压项的模拟值偏低,而赤道向AAM 函数气压项的模拟值偏高,轴向AAM 函数的风项模拟得最好,而赤道向AAM 函数的风项模拟得较差.总之,高精度的天文观测的地球自转系列可以作为全球环流模型检验的一种重要参考依据. 相似文献
6.
地球自转极移近120天准周期变化的小波分析及其大气激发机制 总被引：2，自引：1，他引：1
本文利用小波变换这一新的频谱分析方法研究了地球自转极移近１２０天准周期变化的时频特征，证实了在极移序列中存在显著的近１２０天准周期振荡，得到了极移准周期变化的周期与振幅随时间变化的规律．以地球自转动力学为基础，在时域内分析了大气变化对自转极移季节内变化的激发．表明大气激发在本文所研究的频段内是极移短周期变化的主要激发源。并发现在极移近１２０天准周期振荡平静时期，发生ＥＬＮｉｎｏ事件，同时日长变化近１２０天准周期变化增强． 相似文献
7.
顾震年 《中国科学院上海天文台年刊》1996,(17):73-79
本采用国际时间局（BIH）和美国喷气推进实验室（JPL）提供的日长变化序列（LOD）和美国气象中心（NMC）及日本气象厅（JMA）推导出的大气角动量（AAM）来重新检测固体地球和大气之间的季节性差异。从4种滤波序列中发现由AAM推出的LODatm周年变化高于观测的LOD约17％,而LOD的半年振幅变化超出LODatm的约30％。本还讨论了几种因素，例如洋流中季节性变化，气象中的系统误差，平流层风的贡献，核的惯量矩作用，空气质量的重新分布补尝及其他未知的激发源来解释它们之间不平衡，今后10年，在研究角动量不平衡中，将用固体地球－大气－海洋动力学系统来代替简单的固体地球－－大气的两体动力学系统。海洋对这季节性不平衡可能有重要贡献。 相似文献
8.
简要说明了天文地球动力学范畴内所研究的潮汐现象，包括由日月引潮力引起的固体潮、海洋潮、大气潮和由于地球自转轴的极移引起的极潮，以及这些潮汐对地球自转和地球自转的测量产生的效应。重点阐述中国天文学界在这一领域里的研究成果。这些研究涉及潮汐影响地球自转的机制，也就是各种潮汐效应与极移、自转速率变化和章动的关系，包括构建这类关系的理论模型，分析潮汐对它们的影响，利用中国古代丰富的天象记录计算地球自转的长期减慢，计算弹性或滞弹地球的洛夫数，依据某一地球模型计算潮汐效应或章动序列等等。研究也涉及在测量地球自转参数的不同技术中各种潮汐效应对测量结果产生的影响及其改正，并涉及与潮汐有关的观测方法的优化和数据处理过程的改进。最后介绍了中国学者所发现的脉冲星的周期和周期变率测量中的潮汐效应，尽管它们的量级甚微，但不容忽视。 相似文献
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10.
本利用AR谱估计的Marple算法分析了ERP（SHA）序列中的谱结构，地球自转（日长变化和极移）的一些基本周期在谱结构中的存在表明，ERP（SHA）序列伯可靠性以及它在天和地球物理方面的可应用性。本还给出了ERP（SHA）序列的高频变化结果。 相似文献
11.
Many asteroids with a semimajor axis close to that of Mars have been discovered in the last several years. Potentially some of these could be in 1:1 resonance with Mars, much as are the classic Trojan asteroids with Jupiter, and its lesser-known horseshoe companions with Earth. In the 1990s, two Trojan companions of Mars, 5261 Eureka and 1998 VF31, were discovered, librating about the L5 Lagrange point, 60° behind Mars in its orbit. Although several other potential Mars Trojans have been identified, our orbital calculations show only one other known asteroid, 1999 UJ7, to be a Trojan, associated with the L4 Lagrange point, 60° ahead of Mars in its orbit. We further find that asteroid 36017 (1999 ND43) is a horseshoe librator, alternating with periods of Trojan motion. This asteroid makes repeated close approaches to Earth and has a chaotic orbit whose behavior can be confidently predicted for less than 3000 years. We identify two objects, 2001 HW15 and 2000 TG2, within the resonant region capable of undergoing what we designate “circulation transition”, in which objects can pass between circulation outside the orbit of Mars and circulation inside it, or vice versa. The eccentricity of the orbit of Mars appears to play an important role in circulation transition and in horseshoe motion. Based on the orbits and on spectroscopic data, the Trojan asteroids of Mars may be primordial bodies, while some co-orbital bodies may be in a temporary state of motion. 相似文献
12.
Magnetars are the neutron stars with the highest magnetic fields up to 1015–1016 G. It has been proposed that they are also responsible for a variety of extra-galactic phenomena, ranging from giant flares in nearby galaxies to fast radio bursts. Utilizing a relativistic mean field model and a variable magnetic field configuration, we investigate the effects of strong magnetic fields on the equation of state and anisotropy of pressure of magnetars. It is found that the mass and radius of low-mass magnetars are weakly enhanced under the action of the strong magnetic field, and the anisotropy of pressure can be ignored. Unlike other previous investigations, the magnetic field is unable to violate the mass limit of the neutron stars. 相似文献
13.
Time scales of the transition from contact binary systems of the W UMa type to single stars of the blue straggler type are estimated. A model of one-way mass transfer from the primary component to the companion inside a common envelope (Eggen et al.) and a model of a contact binary lying on the zero-age main sequence with a companion that is losing mass (F. van't Veer) are used to calculate these scales. The merging times of components were calculated for 304 contact systems of the W UMa type from the Catalog of Approximate Photometric and Absolute Elements of Eclipsing Variable Stars on a scale of loss of mass and orbital angular momentum due to magnetic braking, under the assumption of synchronization of the axial rotation and orbital revolution. On the basis of the resulting statistics, the characteristic merging scales are 0.4-0.6 and 0.5-0.7 Gyr, respectively, for the above two models. The results of a comparison with the work of other authors are discussed. 相似文献
14.
分析了上两个世纪发生在淮河的洪水事件的可公度性，根据其可公度值及其黄金分割点指出1991年与2003年淮河洪水的不可避免，最后讨论了可公度性的局限及淮河洪水可公度值的可能机制。 相似文献
15.
We present a numerical method for inverting long-period components of lightcurves of asynchronous binary asteroids. Data of five near-Earth binary asteroids, (175706) 1996 FG3, (65803) Didymos, (66391) 1999 KW4, (185851) 2000 DP107 and (66063) 1998 RO1, for two of them from more than one apparition, were inverted. Their mutual orbits' poles and Keplerian elements, size ratios, and ellipsoidal shape axial ratios were estimated via this inversion. The pole solutions and size ratios for 1999 KW4 and 2000 DP107 are in a good agreement with independent estimates from radar measurements. We show that uncertainties of estimates of bulk densities of binary systems can be large, especially when observed on short arcs. 相似文献
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Influences of the mass, moment of inertia, rotation, absence of stability in the atmosphere and some other parameters of neutron stars on the evolution of pulsars are examined. It is shown that the locations and evolutions of soft gamma repeaters, anomalous X-ray pulsars and other types of pulsar on the period versus period derivative diagram can be explained adopting values of B < 1014 G for these objects if they have smaller mass (e.g. about 0.5 Solar mass) compared to the conventionally adopted values of mass. This approach gives the possibility to explain many properties of different types of pulsar. 相似文献
18.
Pavel Mayer Marek Wolf P. G. Niarchos K. D. Gazeas V. N. Manimanis Drahomír Chochol 《Astrophysics and Space Science》2006,304(1-4):39-41
New precise times of minimum light for several early-type eclipsing binaries were obtained at three observatories. The changes of period of the following measured binaries are discussed: V1182 Aql, LY Aur, SZ Cam, FZ CMa, QZ Car, LZ Cen, V606 Cen, AH Cep and TU~Mus. 相似文献
19.
This paper deals with the observed variation in the flattening of galaxies with the density of galaxies in the subclusters
of Coma surrounding NGC 4889, NGC 4874, and NGC 4839 based on data from the Abastumani Combined Catalog of Galaxies. The mean
values of the observed ratios of the diameters of the galaxies, as well as histograms of their distributions, indicate that
in the central, dense regions of the subclusters within a volume of 0.5h
75
−1
Mpc3, E and S0 type galaxies are close to spheroidal. A significant reduction in the mean values of the diameters of the galaxies
in the subclusters is noted, regardless of their morphology relative to the galaxies in the halo of the Coma cluster. In the
subclusters, spiral galaxies are found with a hydrogen deficit that is more than 5 times the hydrogen deficit in spirals within
the halo of the cluster. According to their 3-D coordinates, most of the galaxies with a hydrogen deficit are located closer
to the south-east edge of the subcluster surrounding NGC 4874 near an extended gas filament in the x-ray region. This may
indicate that the subcluster is moving toward a central condensation of faint galaxies in the Coma cluster and a possible
merger with it.
__________
Translated from Astrofizika, Vol. 50, No. 3, pp. 355–368 (August 2007). 相似文献