Generation Mechanism of Electromagnetic Rising-tone Emissions in the Magnetosphere

Yoshiharu Omura

2014

Abstract

The We describe the generation mechanism of electromagnetic waves known as whistler-mode chorus emissions with right-handed polarization and electromagnetic ion cyclotron (EMIC) triggered emissions with left-handed polarization interacting with energetic electrons and protons, respectively, through cyclotron resonance. These waves are frequency observed in the magnetospheres of the magnetized planets such as Earth, Jupiter, and Saturn. They are coherent waves with increasing frequencies generated at the magnetic equator and propagating along the magnetic field. The resonant particles undergo nonlinear trapping motion around the resonance velocity, and they form electromagnetic electron/ion holes in the velocity phase space. In the presence of the inhomogeneity due to the frequency variation and the gradient of the magnetic field, the electron holes or hills result in resonant currents generating rising-tone emissions [1,2,3]. After formation of a coherent wave at a frequency of the maximum linear growth rate, triggering of nonlinear wave growth with the increasing frequency takes place when the wave amplitude is close to the optimum wave amplitude [4,5]. The wave amplitude also has to be greater than the threshold amplitude [2,3] so that the nonlinear wave growth can occur as an absolute instability at the magnetic equator. The triggering process is repeated at progressively higher frequencies, generating subpackets of a rising-tone element. These electromagnetic emissions control the dynamics of radiation belts. Whistler-mode chorus emissions are responsible for acceleration of relativistic electrons [6,7,8], while EMIC triggered emissions induces precipitation of relativistic electrons into the atmosphere through anomalous cyclotron resonance [9,10].

References

1. [9] Y. Omura and Q. Zhao, Nonlinear pitch-angle scattering of relativistic electrons by EMIC waves in the inner magnetosphere, Journal of Geophysical Research, 117, A08227, 2012.
2. [10] Y. Omura and Q. Zhao, Relativistic electron microbursts due to nonlinear pitch-angle scattering by EMIC triggered emissions, Journal of Geophysical Research, 118, pp. 5008-5020, 2013.

Paper Citation

in Harvard Style

Omura Y. (2014). Generation Mechanism of Electromagnetic Rising-tone Emissions in the Magnetosphere . In Proceedings of the Third International Conference on Telecommunications and Remote Sensing - Volume 1: ICTRS, ISBN 978-989-758-033-8, pages 121-122. DOI: 10.5220/0005422201210122

in Bibtex Style

@conference{ictrs14,
author={Yoshiharu Omura},
title={Generation Mechanism of Electromagnetic Rising-tone Emissions in the Magnetosphere},
booktitle={Proceedings of the Third International Conference on Telecommunications and Remote Sensing - Volume 1: ICTRS,},
year={2014},
pages={121-122},
publisher={SciTePress},
organization={INSTICC},
doi={10.5220/0005422201210122},
isbn={978-989-758-033-8},
}

in EndNote Style

TY - CONF
JO - Proceedings of the Third International Conference on Telecommunications and Remote Sensing - Volume 1: ICTRS,
TI - Generation Mechanism of Electromagnetic Rising-tone Emissions in the Magnetosphere
SN - 978-989-758-033-8
AU - Omura Y.
PY - 2014
SP - 121
EP - 122
DO - 10.5220/0005422201210122