Line Shape of Optical Satellites in a Magnetized Turbulent Plasma

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概要

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• Consideration is given on tlte shape of the allowed and satellite lines in thespectra of radiation emitted by a He-like radiator in a magnc:tized turbulentplasma. The satellite is considcred to be induced by a high-freqx.uency, coherentand spatially inhomogeneous electric field oscillating in the direction parallel orperpendicular to the static magnetic field. The frequency of fine electric fieldis supposed to be near-resona?at to the interval between upper 1.wo levels. Theeffects of degeneracy and the magnetic field are treated exactly. Numerical calcu-Nations are presented for a $et of levels n."D, n."P and nt"S (n.=3, 4, 5, 6, ng='2.).For the linearly polarized elect:ric field perpendicular to the magnetic field, somezer'o points and gaps appear in the satellite which are not expectant in the case ofthe circularly polarized electric field.

• 社団法人日本物理学会の論文
• 1980-05-15

著者

• Mizuta Yo

  Department Of Physics Faculty Of Science Hokkaido University

関連論文

• Stochastic Theory of He I Satellite Line Shape in a Plasma
• Optical Satellites of Langmuir Turbulence
• Line Shape of Optical Satellites in a Magnetized Turbulent Plasma
• On the Behaviour of the Polyatomic Chain as the Harmonic Heat Reservoir

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