Acceleration mechanism of particles in the Type-I cometary plasma |
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| Authors: | Li Zhongyuan Guo Sheyu |
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| Affiliation: | (1) International Centre for Theoretical Physics, Trieste, Italy;(2) Present address: Department of Earth and Space Science, University of Science and Technology, Hefei, China;(3) Present address: Institute of Plasma Physics, Heifei, China |
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| Abstract: | ![]()
In the paper, the accelerated effect of ions has been discussed. The transversal magnetic disturbance is able to bring about the magnetic annihilation and merge in some cometary area. The non-steady-state reconnection process can transform the magnetic energy of some cometary area into the kinetic energy of plasma. In addition, the  two stream instability caused by both solar wind and cometary plasmas exists in Type-I tail, it can also lead the paticles to be accelerated and heated in the plasma tail. |
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