It is well known that accretion disks are hydrodynamic disks with anomalous viscosity. 天体物理吸积盘是具有反常粘滞的流体盘。
In this thesis, using the new model of anomalous viscosity, we discuss the structure of magnetized thin accretion disks, the magnetic instability in the accretion disks and. 本文主要利用这种全新的反常黏滞机制,讨论了磁化薄吸积盘的结构、吸积盘的磁不稳定性以及反常耗散对磁旋转不稳定性的影响。
Because of the anomalous viscosity, the I-mode is always unstable in the inner disk. 由于反常粘滞的存在,导致I-mode在盘的内区是始终不稳定的。
The stationary vertical structure of a thin disk around a black hole is considered with the anomalous magnetic viscosity~ ( [ 1]). 利用反常粘滞[1]研究了黑洞周围薄吸积盘的静态垂向结构。
An accretion disk with vertical structure is studied by using a new anomalous viscosity. 利用一种全新的反常粘滞,主要研究了具有垂向结构的吸积盘。
Using the anomalous viscosity ( Li& Zhang 2002), we discuss the stationary vertical structure of a thin disk around a black hole. 我们利用磁吸积盘一种全新的反常粘滞结果(Li&Zhang2002),研究了黑洞周围薄吸积盘的静态垂向结构。
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。