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Precipitation of trapped relativistic electrons by amplified whistler waves in the magnetosphere
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10.1063/1.2743618
/content/aip/journal/pop/14/6/10.1063/1.2743618
http://aip.metastore.ingenta.com/content/aip/journal/pop/14/6/10.1063/1.2743618
View: Figures

Figures

Image of FIG. 1.
FIG. 1.

Momentum distribution of energetic electrons and the regions close to cyclotron resonant interaction with the wave.

Image of FIG. 2.
FIG. 2.

Temporal evolution of the amplitude of a whistler wave traversing the magnetosphere.

Image of FIG. 3.
FIG. 3.

Amplitude gain of the amplified whistler wave as a function of the density of energetic electrons .

Image of FIG. 4.
FIG. 4.

The dependency of the peak intensity and the modulation period of an amplified wave on the intensity of the incident wave.

Image of FIG. 5.
FIG. 5.

Amplitude gain of the amplified whistler wave as a function of the intensity of the incident whistler wave.

Image of FIG. 6.
FIG. 6.

(Color online) Temporal evolution of the pitch angle of a electron, which is interacting with a whistler wave at Doppler shifted cyclotron resonance. The wave magnetic field increases consecutively from 1 to .

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/content/aip/journal/pop/14/6/10.1063/1.2743618
2007-06-27
2014-04-23
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Precipitation of trapped relativistic electrons by amplified whistler waves in the magnetosphere
http://aip.metastore.ingenta.com/content/aip/journal/pop/14/6/10.1063/1.2743618
10.1063/1.2743618
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