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celestial mechanics相关的网络例句

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与 celestial mechanics 相关的网络例句 [注:此内容来源于网络,仅供参考]

Celestial mechanics enables astronomers to calculate the positions of the planets at any time in the post or future and to predict the movements of comets.

天体力学使文学家能计算出行星在过去或将来任何时候的位置,并能预报彗星的运行位置。

See [90]. The theoretical work by these mathematicians supplied many of the ideas and approaches that were later used in more applied situations in physics, celestial mechanics, chemistry, biology, and other fields.

这些数学家的理论工作提供了很多思想和方法,这些后来都被应用于物理、天体力学、化学、生物学和其它领域更为复杂的情形。

The study of the mathematical model for such motion is called celestial mechanics , and involves a finite number of bodies moving under the effects of gravitational attraction given by the Newtonian laws.

对于这种运动的数学模型的研究称作天体力学,包括研究在牛顿万有引力定律作用下的有限个天体的运动。

Celestial mechanics: numerical method, N-body simulation; planetary systems: Solar System

天体力学:数值算法,N体模拟;行星系统:太阳系

At that time, however, nonlinear differential equations had no universal solutions and some problems of celestial mechanics were still required to be resolved.

而非线性微分方程没有普遍解法以及一些天体力学问题的未决,促使庞加莱在微分方程求解过程中引入定性思想,创立了常微分方程实域定性理论这一新分支,突破了原有的微分方程求解的思维束缚,是微分方程研究历史上的一次重大飞跃。

Furthermore the laws of celestial mechanics www.readinggroupguides.com/ credited to Copernicus, Kepler and Galileo were know by the Chinese and used to create a very accurate calender in 1280 for Kublai Khan (page 23 -28) that was later adopted by the Europeans.

此外天体力学定律 www.readinggroupguides.com/贷记哥白尼,开普勒和伽利略系统是由中国的了解和用于创建一个非常准确的在1280年忽必烈汗(页日历23 -28),后来由欧洲人通过。

This problem, which was certainly known to the ancients, became especially acute in the seventeenth century with the invention of celestial mechanics, which first gave philosophers a certain picture of a way the world might be: it might be a world whose future states were entirely determined by the past and the laws of nature (of which Newton's laws of motion and law of universal gravitation served as paradigms).

这个从很早就被知道的问题,在十七世纪之后变得尖锐起来,因为引力力学第一次给予了哲学家一个明确的世界图景:可能世界的未来事态完全可以被过去和自然律(Newton的运动律和万有引力定律是范例)所决定。

Birkhoff, Siegel, Kolmogorov, Arnold, Moser, Herman, and many others investigated the ideas of stability and found complicated behavior for systems arising in celestial mechanics and other such physical systems, which could be described by what are called Hamiltonian differential equations .

Birkhoff , Siegel , Kolmogorov , Arnold , Moser , Herman 和其他很多研究者研究稳定性的思想,发现了具有复杂行为的系统出现在天体力学和其它相似的物理系统中,这些都可以用称为 Hamilton 微分方程来描述。

Based on the ISC earthquake catalogue data, according to the orbit equations of two-body-problem and the perturbation theory of celestial mechanics, we could determine the projection pole of the sun, and thus calculate the zenith distance from the sun to the epicenter. After calculating all the earthquakes on their zenith distances, we could get the distribution of the solar zenith distance versus the occurring probability of earthquakes.

基于ISC地震记录,利用天体动力学中二体问题的轨道方程和摄动理论,确定发震时刻太阳在地面的投影点位置,并进一步计算出太阳相对震中的地心天顶距,将地震按天顶距的大小进行统计,得到地震的太阳天顶距地震频度分布。

The second-order post-Newtonian(2PX) equations of light ray have to be discussed under the recent extension of the DSX scheme which was founded in early 1990's to discuss a complete first-order post-Newtonian celestial mechanics for N arbitrarily composed and shaped, rotating deformable bodies.

DSX体系是在20世纪90年代初建立的,用来讨论对N个任意形状和组成、自转可变形物体的一套完整的一阶后牛顿(1PN)天体力学理论。

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