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- W2049880917 abstract "We propose to answer the question as to whether there could be a topological configuration of the magnetic field, velocity field, and a potential field which could retain the galactic plasma in the spiral arm in a self-consistent way. In the kinematic theory we have developed here, we do not have an external magnetic field such as an intergalactic field, but have only the internal magnetic fields generated by the motion of the plasma as such. We have applied the kinetic equations to a galactic plasma rather than the fluid equations as is usually done; and, assuming a general quadratic expression for the distribution function in the velocity space, we have looked for the complete class of self-consistent magnetic fields, potential fields, as well as density distributions. Many important features of the magnetic fields are brought out and discussed at length. It is found that the frozen-in condition is valid for such a low-density plasma as well (eq. [4.11]). We have also indicated the lines in which this theory could be developed further." @default.
- W2049880917 created "2016-06-24" @default.
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- W2049880917 date "1968-06-01" @default.
- W2049880917 modified "2023-09-25" @default.
- W2049880917 title "Dynamics of galactic plasma. I" @default.
- W2049880917 doi "https://doi.org/10.1139/p68-447" @default.
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