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Electrostatic ion-acoustic-like instabilities in the solar wind with a backstreaming alpha particle beam
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10.1063/1.3431631
/content/aip/journal/pop/17/6/10.1063/1.3431631
http://aip.metastore.ingenta.com/content/aip/journal/pop/17/6/10.1063/1.3431631

Figures

Image of FIG. 1.
FIG. 1.

Nonlinear dispersion relation [Eq. (2)], vs , for , , , and corresponding to , for (a) , (b) , (c) , and (d) .

Image of FIG. 2.
FIG. 2.

Nonlinear dispersion relation [Eq. (2)], vs for , , , , , and corresponding to , for (a) , (b) , (c) , (d) , (e) , (f) , and (g) the same as (a), but for .

Image of FIG. 3.
FIG. 3.

Three dimensional plot for the nonlinear dispersion relation, Eq. (2). The -coordinate represents , while the -coordinate represents . The parameters are , , , , , , , and . This figure is the same case of Fig. 2(g), showing on the plane the instabilities and in the third coordinate [] the growth rates of the instabilities. Thus, the plane , is just the same as Fig. 2(g).

Image of FIG. 4.
FIG. 4.

Maximum growth rate vs finite amplitude wave amplitude , for and , , , and .

Image of FIG. 5.
FIG. 5.

Maximum growth rate with vs , for , and with (a) , (b) , (c) , and (d) .

Image of FIG. 6.
FIG. 6.

Nonlinear dispersion relation [Eq. (2)], vs , for , , , , , , , , for . The arrows show and .

Image of FIG. 7.
FIG. 7.

Linear dispersion relation [Eq. (1)] for , , , and , showing that for there is no solution for in the first quadrant of the figure.

Tables

Generic image for table
Table I.

Summary of the various electrostatic instabilities in an alpha particle backstreaming solar wind and in counterstreaming alpha particle-proton beams.

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/content/aip/journal/pop/17/6/10.1063/1.3431631
2010-06-11
2014-04-20
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Electrostatic ion-acoustic-like instabilities in the solar wind with a backstreaming alpha particle beam
http://aip.metastore.ingenta.com/content/aip/journal/pop/17/6/10.1063/1.3431631
10.1063/1.3431631
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