Some discussion on the acceleration mechanism of particles in the type-I plasma comet

Physics

Scientific paper

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Comet Tails, Giacobini-Zinner Comet, Magnetic Fields, Particle Acceleration, Magnetic Field Reconnection, Plasmas (Physics), Turbulence

Scientific paper

Earlier, the large acceleration of plasma (300 cm/sq s) were already observed in type-I tail. Recently, the direct measurements for comet G-Z showed that the energy of particle reaches 2x105 eV, an energy much higher than the initial energy of comet particles (less than or = 2x104 eV). So there should be an accelerated process in the comet.

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