keplerian

keplerian

1. 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

2. Keplerian telescope

开普勒式望远镜 开普勒望远镜

3. 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。

4. Keplerian ellipse

开普勒轨道

5. Keplerian motion

开普勒运动

6. 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.

7. 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。

8. 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；

9. 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;

10. keplerian cllipse

轨道椭圆

11. 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;