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月球作为一个既没有全球性磁场又没有明显大气层的星体,一直以来都认为太阳风是直接作用在月球向阳面且被完全吸收。然而近年来,越来越多的观测与模拟结果表明,太阳风与月表的相互作用由于月表局地磁异常的存在而出现一些”例外”,在一定条件下,可以形成月表微磁层(LMM)。
Motivated by observations that only a very few stars have been found to have antisolar differential rotation, much weaker in amplitude than that of the Sun, we analyze the stability of antisolar and s...
Magnetic fields in the intra-cluster medium of galaxy clusters have been studied in the past years through different methods. In the next years the up-coming generation of radio telescopes is going to...
Recently, secondary island formation due to the tearing instability of the Sweet-Parker current sheet was identified as a possible mechanism that can lead to fast reconnection (less sensitive dependen...
Sunspot fine structure has been modeled in the past by a combination of idealized magneto-convection simulations and simplified models that prescribe the magnetic field and flow structure to a large d...
Context. Oscillations in coronal loops are usually interpreted in terms of uncoupled magnetohydrodynamic (MHD) waves. Examples of these waves are standing transverse motions, interpreted as the kink M...
The possible role of magneto-rotational instability (MRI) and its driven MHD turbulence in the solar interior is studied on the basis of the linear and nonlinear theories coupling with physical para...
Parker instability arises from the presence of magnetic fields in a plasma such as the interstellar medium (ISM),wherein the magnetic buoyant pressure expels the gas and causes the gas to move along t...
The ICM has been suggested to be buoyantly unstable in the presence of magnetic field and anisotropic thermal conduction. We perform first cosmological simulations of galaxy cluster formation that sim...
MHD Driving of Relativistic Jets。
The MHD Collapsar Model for GRBs:an Inflow produces an Outflow。
MHD Stabiblity of a Solar Prominence Embedded in an External Vertical Magnetic Field。
Binary star formation and mass outflows:Mhd nested grid simulation。
Evolution of protoplanetary discs driven by MHD turbulence and other agents。
MHD ionization fronts     MHD  ionization fronts       2009/6/11
MHD ionization fronts。

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