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Heating of the background plasma by obliquely propagating Alfven waves excited in the electromagnetic alpha/proton instability
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10.1063/1.3693373
/content/aip/journal/pop/19/3/10.1063/1.3693373
http://aip.metastore.ingenta.com/content/aip/journal/pop/19/3/10.1063/1.3693373
View: Figures

Figures

Image of FIG. 1.
FIG. 1.

The time evolution of (a) the amplitude of the fluctuating magnetic field , (b) the relative drift speed between protons and alpha particles .

Image of FIG. 2.
FIG. 2.

(Color online) The contour of the characteristics of diagram obtained from the FFT transforming of at , , and .

Image of FIG. 3.
FIG. 3.

(Color online) The contour of the spectrum evolution of the wave frequencies obtained from the average value of the wavelet power spectrum of the time series of at 100 selected grids.

Image of FIG. 4.
FIG. 4.

The time evolution of amplitude of the fluctuating magnetic field (where ) and .

Image of FIG. 5.
FIG. 5.

The time evolution of (a) the parallel temperature and perpendicular temperature of the alpha component, (b) the parallel temperature and perpendicular temperature of the proton component. Dashed lines represent the parallel temperatures, and solid lines represent the perpendicular temperatures.

Image of FIG. 6.
FIG. 6.

The scatter plots of alpha particles in the ( , ) at different times.

Image of FIG. 7.
FIG. 7.

The scatter plots of protons in the ( , ) space at different times.

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/content/aip/journal/pop/19/3/10.1063/1.3693373
2012-03-15
2014-04-16
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Heating of the background plasma by obliquely propagating Alfven waves excited in the electromagnetic alpha/proton instability
http://aip.metastore.ingenta.com/content/aip/journal/pop/19/3/10.1063/1.3693373
10.1063/1.3693373
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