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Polarizations of coupling kinetic Alfvén and slow waves
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10.1063/1.3609782
L. Chen1,2,a) and D. J. Wu1,b)
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Affiliations:
1 Purple Mountain Observatory, CAS, Nanjing 210008, China
2 Graduate School, CAS, Beijing 100012, China
a) Electronic mail: clvslc214@pmo.ac.cn.
b) Author to whom correspondence should be addressed. Electronic mail: djwu@pmo.ac.cn.
Phys. Plasmas 18, 072110 (2011)
/content/aip/journal/pop/18/7/10.1063/1.3609782
http://aip.metastore.ingenta.com/content/aip/journal/pop/18/7/10.1063/1.3609782
View: Figures

## Figures

FIG. 1.

The electromagnetic polarizations versus the perpendicular wavenumber: Panels, from the top down, present , , and , respectively, where the dashed lines plot the corresponding ideal MHD solutions for the sake of comparison and the left and right columns correspond to the cases of Alfvén and slow modes, respectively. The fixed parameters , , and have been used.

FIG. 2.

The electromagnetic polarizations versus the perpendicular wavenumber: Panels, from the top down, present , , and , respectively, where the dashed lines plot the corresponding ideal MHD solutions for the sake of comparison and the left and right columns correspond to the cases of Alfvén and slow modes, respectively. The fixed parameters , , and have been used.

FIG. 3.

The electromagnetic polarizations versus the temperature ratio of ion to electron : Panels, from the top down, present , , and , respectively, where the dashed lines plot the corresponding ideal MHD solutions for the sake of comparison and the left and right columns correspond to the cases of Alfvén and slow modes, respectively. The fixed parameters , , and have been used.

FIG. 4.

The electromagnetic polarizations versus the temperature ratio of ion to electron : Panels, from the top down, present , , and , respectively, where the dashed lines plot the corresponding ideal MHD solutions for the sake of comparison and the left and right columns correspond to the cases of Alfvén and slow modes, respectively. The fixed parameters , , and have been used.

FIG. 5.

The electromagnetic polarizations versus the plasma parameter: Panels, from the top down, present , , and , respectively, where the dashed lines plot the corresponding ideal MHD solutions for the sake of comparison and the left and right columns correspond to the cases of Alfvén and slow modes, respectively. The parameters , , and have been used.

FIG. 6.

The electromagnetic polarizations versus the plasma parameter: Panels, from the top down, present , , and , respectively, where the dashed lines plot the corresponding ideal MHD solutions for the sake of comparison and the left and right columns correspond to the cases of Alfvén and slow modes, respectively. The parameters , , and have been used.

/content/aip/journal/pop/18/7/10.1063/1.3609782
2011-07-22
2014-04-20

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