27–31 Oct 2025
InterContinental Chengdu Global Center
Asia/Shanghai timezone
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Gyrating Ion Beam Driven Whistler Wave Instability in a Dusty Plasma

TUAO02
28 Oct 2025, 09:20
20m
InterContinental Chengdu Global Center

InterContinental Chengdu Global Center

Chengdu, China
Contributed Oral Presentation Cyclotron and Technology Cyclotron and Technology (1)

Speaker

Amit kumar (Amity University)

Description

This manuscript examines the non-linear interaction between the negative energy beam cyclotron mode and high-frequency whistler waves. The negative energy beam mode is supported in the vicinity of the beam gyro-frequency harmonics by a gyrating ion beam with
ring shaped velocity distribution. Using a gyrating ion beam, we have examined how dust charge variations affect the parametric up-conversion of high frequency whistler waves (WW) into an side band wave and a low-frequency mode. For the linked modes, a non-linear dispersion relation is obtained. It is demonstrated that whistler waves divided by beam gyro-frequency harmonics are up-converted by a gyrating ion-beam frequency. A formula for the ion cyclotron mode wave growth rate has been obtained. The estimation of the turbulence growth rate takes into account for the typical parameters of an existing dusty plasma. It is detected that an increased growth rate appears with a rise in the pump wave amplitude, beam gyro-frequency, number density of dust grains, and the relative density of dust grains. However, a decline in the growth rate has been detected with increasing gyrating ion beam density and dust grains size.

Authors

Amit kumar (Amity University) Mrs Twinkle Pahuja (Amity University)

Presentation materials

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