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Fig. 6. | Earth, Planets and Space

Fig. 6.

From: Narrowband frequency-drift structures in solar type IV bursts

Fig. 6.

Calculated wave-dispersion relation based on the Appleton-Hartree equation for Ļ‰p/Ļ‰ce = 10, fp = Ļ‰p/2p = 325 MHz and Īø = 0Ā°. The solid line shows L-O mode wave, the dotted line does Langmuir wave, and the dashed line does whistler-mode wave. The arrows on the graph indicate the solution of the non-linear three-wave interaction, L + w ā†’ T, for whistler-mode waves of 0.25Ļ‰ce.

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