keplerian
音標發(fā)音
- 美式音標 [kep?li?ri?n]
- 國際音標 [kep'li?ri?n]
- 英式發(fā)音
基本解釋
- adj.（德國天文學家）開普勒的，開普勒定律的，開普勒理論的
英漢例句
- Using the new ?anomalous magnetic Prandtl number? in accretion disks, we study the effect of dissipation on magnetic instability of Keplerian disks.
我們利用吸積磐中新的反常磁普朗特數(shù)來研究耗散過程對開普勒磐磁不穩(wěn)定性的影響. - A group of relative motion equations were given with the Keplerian motion assumption,which was proved to be true in physical concept.
針對圓形軌道串行衛(wèi)星編隊進行研究,推導出滿足開普勒軌道假設的相對運動方程,從物理概唸上証明了這種描述關系的正確性; - 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數(shù)的基礎上，我們研究了耗散過程對開普勒磐磁不穩(wěn)定性的影響。 - In Keplerian disks, the magnetic field is smaller, the dissipation caused by anomalous viscosity and anomalous resistivity deviates from the ideal more greatly.
開普勒磐中,磁場越小,由反常粘滯及反常阻抗引起的耗散偏離理想情況就越大。 - 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.
廻顧了重力測量和衛(wèi)星重力探測技術的發(fā)展和應用，闡述了描述低軌衛(wèi)星狀態(tài)的直角坐標、Kepler根數(shù)、Hill根數(shù)和Equinoctial根數(shù)之間的相互關系，認爲Hill根數(shù)和Equinoctial根數(shù)能夠避免由衛(wèi)星軌道奇異帶來的計算問題，分析了低軌衛(wèi)星的受攝運動，給出了攝動模型。