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131.
Yann Alibert Christoph Mordasini Olivier Mousis Willy Benz 《Space Science Reviews》2005,116(1-2):77-95
We present models of giant planet formation, taking into account migration and disk viscous evolution. We show that migration
can significantly reduce the formation timescale bringing it in good agreement with typical observed disk lifetimes. We then
present a model that produces a planet whose current location, core mass and total mass are comparable with the one of Jupiter.
For this model, we calculate the enrichments in volatiles and compare them with the one measured by the Galileo probe. We
show that our models can reproduce both the measured atmosphere enrichments and the constraints derived by Guillot et al. (2004), if we assume the accretion of planetesimals with ices/rocks ratio equal to 4, and that a substantial amount of CO2 was present in vapor phase in the solar nebula, in agreement with ISM measurements. 相似文献
132.
简要介绍了军用飞机飞行品质MIL—STD—1797A中有关俯仰轴频域难则的要求和原由。提出了对这些难则的理论计算和模拟试验方法。并以某飞机为例,利用所提出的方法,对其飞行品质进行了计算和模拟。结果表明,所提出的计算和模拟方法是合理的。最后,讨论了驾驶员模型形式对俯仰轴飞行品质的影响。 相似文献
133.
对PIO预测的A值及A准则的分析 总被引:1,自引:0,他引:1
从应用的角度详细地介绍了国外预测PIO时使用A值及A准则的情况。进行了计算公式的推导,讨论了准则在推导过程中所采用的假设及其适用情况,重新整理和校核了计算步骤和算例,以便于推广使用。 相似文献
134.
Bruno Sicardy 《Space Science Reviews》2005,116(1-2):457-470
Planetary rings are found around all four giant planets of our solar system. These collisional and highly flattened disks
exhibit a whole wealth of physical processes involving dust grains up to meter-sized boulders. These processes, together with
ring composition, can help understand better the formation and evolution of proto-satellite and proto-planetary disks in the
early solar system. The present chapter reviews some fundamental aspects of ring dynamics and composition. The forthcoming
exploration of the Saturn system by the Cassini mission will bring both high resolution and time-dependent information on Saturn’s rings. 相似文献
135.
H.-E. Frhlich V. Müller H. Oleak 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
Dusty pregalactic Population III objects may provide a mechanism for an effective thermalization of the star radiation. They may generate the observed microwave background and so the high cosmic photon entropy. Assuming a tepid universe a smaller primordial entropy contribution results in reasonable mass scales and amplification factors of pregalactic density fluctuations. 相似文献
136.
David N. Schramm 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
To illustrate the interaction of Grand Unified Theories (GUTs), supersymmetry (SUSY), and cosmology, a worked example is carried out. This example is the dark matter problem, or “What is the dominant matter of the Universe?” It is shown that if GUTs are assumed then the primordial perturbations are probably adiabatic, if inflation is assumed then Ω = 1 and GUTs first name is probably SUSY. If Ω = 1, big bang nucleosynthesis tells us that the bulk of the matter is non-baryonic. SUSY-GUTs gives us some possible candidate inos to which massive neutrinos, axion or planetary mass black holes can be added. These candidates can be classified hot (or warm) or cold types of dark matter. It is shown that hot gives Ω = 1 and naturally gives large scale structure but does not give small scale structure or galaxy formation times, whereas cold gives small scale structure and formation times but cannot easily yield Ω = 1. It is concluded that either a hybrid of both hot and cold or non-random phases for the perturbations may be needed. 相似文献
137.
Guido Chincarini 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
In this lecture I review part of the published and unpublished observational evidence showing that cluster spiral galaxies are hydrogen deficient. Always using observational data, it is argued that the deficiency is due to the interaction between the galaxies and the intergalactic medium. Furthermore it is shown that the stellar population of deficient galaxies has also been affected and a brief discussion is given of the mechanisms at work. 相似文献
138.
139.
本文采用近似的激波关系、球锥体压力分布、平衡气体状态方程、边界层厚度计算公式及转捩准则等,按照流管法计算了4种再入飞行器的外流转捩雷诺数和转捩距离,并给出了高硅氧、碳石英、碳碳球锥模型的转捩雷诺数范围,对再入飞行器和模型的计算结果作了分析和比较。 相似文献
140.
P.E.J. Nulsen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
Rapidly cooling gas is commonly found near the centres of clusters of galaxies. The structure of the resulting gas flows is reviewed. Total gas cooling rates of several hundred M yr−1 have been observed in a number of cases. Thermal instability and the ultimate fate of the cooled gas are discussed. The cooled gas could easily have formed a massive central galaxy. 相似文献