Radio Radiation Mechanism of Two-Streams Plasma in the Astrophysical Jet
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Abstract
To explain the radio mechanism of non-relativistic jets, we investigate a nonlinear process in which ion-acoustic waves scatter into high frequency electromagnetic waves by the plasma having a non-Maxwell distribution with non-relativisical energetic electrons. The calculated reaults show that this mechanism is efficient, and may apply to the radiation of jets from active galaxies and radio bursts of sun flares.
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LU Shengzhi, TONG Yi, SU Yang. Radio Radiation Mechanism of Two-Streams Plasma in the Astrophysical Jet[J]. Chin. Phys. Lett., 1995, 12(3): 189-192.
LU Shengzhi, TONG Yi, SU Yang. Radio Radiation Mechanism of Two-Streams Plasma in the Astrophysical Jet[J]. Chin. Phys. Lett., 1995, 12(3): 189-192.
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LU Shengzhi, TONG Yi, SU Yang. Radio Radiation Mechanism of Two-Streams Plasma in the Astrophysical Jet[J]. Chin. Phys. Lett., 1995, 12(3): 189-192.
LU Shengzhi, TONG Yi, SU Yang. Radio Radiation Mechanism of Two-Streams Plasma in the Astrophysical Jet[J]. Chin. Phys. Lett., 1995, 12(3): 189-192.
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