Plasma maser interaction with magnetohydrodynamic wave turbulence

M. Nambu; T. Hada; T. Terasawa; K. S. Goswami; S. Bujarbarua

doi:10.1088/0031-8949/47/3/012

Plasma maser interaction with magnetohydrodynamic wave turbulence

M. Nambu, T. Hada, T. Terasawa, K. S. Goswami, S. Bujarbarua

Research output: Contribution to journal › Article › peer-review

4 Citations (Scopus)

Abstract

The energy up-conversion from the kinetic Alfven wave turbulence to the ordinary mode radiation through the plasma-maser process is studied. Thegrowth rate of the ordinary mode originates from two mode-mode coupling terms, viz: The direct and polarization terms. In contrast to the previous electrostatic wave case, both contributions give large growth rate forthe ordinary mode radiation. The results have potential importance tointerpret numerous astrophysical radio phenomena, because the magnetohydrodynamic (MHD) waves contain the dominant turbulent fluctuationsin astrophysical plasmas.

Original language	English
Pages (from-to)	419-427
Number of pages	9
Journal	Physica Scripta
Volume	47
Issue number	3
DOIs	https://doi.org/10.1088/0031-8949/47/3/012
Publication status	Published - Mar 1 1993

All Science Journal Classification (ASJC) codes

Atomic and Molecular Physics, and Optics
Mathematical Physics
Condensed Matter Physics
Physics and Astronomy(all)

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10.1088/0031-8949/47/3/012

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abstract = "The energy up-conversion from the kinetic Alfven wave turbulence to the ordinary mode radiation through the plasma-maser process is studied. Thegrowth rate of the ordinary mode originates from two mode-mode coupling terms, viz: The direct and polarization terms. In contrast to the previous electrostatic wave case, both contributions give large growth rate forthe ordinary mode radiation. The results have potential importance tointerpret numerous astrophysical radio phenomena, because the magnetohydrodynamic (MHD) waves contain the dominant turbulent fluctuationsin astrophysical plasmas.",

author = "M. Nambu and T. Hada and T. Terasawa and Goswami, {K. S.} and S. Bujarbarua",

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AU - Nambu, M.

AU - Hada, T.

AU - Terasawa, T.

AU - Goswami, K. S.

AU - Bujarbarua, S.

PY - 1993/3/1

Y1 - 1993/3/1

N2 - The energy up-conversion from the kinetic Alfven wave turbulence to the ordinary mode radiation through the plasma-maser process is studied. Thegrowth rate of the ordinary mode originates from two mode-mode coupling terms, viz: The direct and polarization terms. In contrast to the previous electrostatic wave case, both contributions give large growth rate forthe ordinary mode radiation. The results have potential importance tointerpret numerous astrophysical radio phenomena, because the magnetohydrodynamic (MHD) waves contain the dominant turbulent fluctuationsin astrophysical plasmas.

AB - The energy up-conversion from the kinetic Alfven wave turbulence to the ordinary mode radiation through the plasma-maser process is studied. Thegrowth rate of the ordinary mode originates from two mode-mode coupling terms, viz: The direct and polarization terms. In contrast to the previous electrostatic wave case, both contributions give large growth rate forthe ordinary mode radiation. The results have potential importance tointerpret numerous astrophysical radio phenomena, because the magnetohydrodynamic (MHD) waves contain the dominant turbulent fluctuationsin astrophysical plasmas.

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JO - Physica Scripta

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Plasma maser interaction with magnetohydrodynamic wave turbulence

Abstract

All Science Journal Classification (ASJC) codes

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