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- keplerian cllipse 轨道椭圆
- Using the new ?anomalous magnetic Prandtl number? in accretion disks, we study the effect of dissipation on magnetic instability of Keplerian disks. 我们利用吸积盘中新的反常磁普朗特数来研究耗散过程对开普勒盘磁不稳定性的影响.
- A group of relative motion equations were given with the Keplerian motion assumption,which was proved to be true in physical concept. 针对圆形轨道串行卫星编队进行研究,推导出满足开普勒轨道假设的相对运动方程,从物理概念上证明了这种描述关系的正确性;
- In chapter three, on the basis of the new anomalous magnetic Prandtl number in accretion disks, we study the effect of dissipation on magnetic instability of Keplerian disks. 第三章在新的反常磁普朗特数的基础上，我们研究了耗散过程对开普勒盘磁不稳定性的影响。
- In Keplerian disks, the magnetic field is smaller, the dissipation caused by anomalous viscosity and anomalous resistivity deviates from the ideal more greatly. 开普勒盘中,磁场越小,由反常粘滞及反常阻抗引起的耗散偏离理想情况就越大。
- Development and applications of gravimetry and satellite-borne gravimetry are reviewed. Relations among the rectangle coordinates, Keplerian elements, Hillian elements and Equinoctial elements to describe the motion of low earth orbit satellite are given. 回顾了重力测量和卫星重力探测技术的发展和应用，阐述了描述低轨卫星状态的直角坐标、Kepler根数、Hill根数和Equinoctial根数之间的相互关系，认为Hill根数和Equinoctial根数能够避免由卫星轨道奇异带来的计算问题，分析了低轨卫星的受摄运动，给出了摄动模型。
- Line Profile of Relativistic Keplerian Rings in a Massive Halo of Neutrinos 大质量中微子晕内相对论性开普勒环的谱线轮廓
- a recycled neutron star previously in an accreting X-ray binary system which accretes for a long time from a surrounding keplerian disk and spun up to millisecond period. 起源于吸积X射线双星的中子星,通过从伴星吸积物质而加速到毫秒周期;
- in Keplerian disks, the magnetic field is smaller, the dissipation caused by anomalous viscosity and anomalous resistivity deviates from the ideal more greatly; 而且，磁场越小，由反常黏滞及反常阻抗引起的耗散过程对磁不稳定性的影响就越大；
- cllipse head 椭圆封头
- Keplerian ellipse 开普勒轨道
- Keplerian telescope 开普勒式望远镜,开普勒望远镜
- Keplerianadj. (德国天文学家)开普勒的;开普勒定律的;开普勒理论的
- Keplerian motion 开普勒运动
- Keplerian orbit 开普勒轨道
- Keplerian orbits 开普勒轨道
