論文

査読有り
2017年10月

Study of Wave-Particle Interactions for Whistler Mode Waves at Oblique Angles by Utilizing the Gyroaveraging Method

RADIO SCIENCE
  • Yi-Kai Hsieh
  • ,
  • Yoshiharu Omura

52
10
開始ページ
1268
終了ページ
1281
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1002/2017RS006245
出版者・発行元
AMER GEOPHYSICAL UNION

We investigate the properties of whistler mode wave-particle interactions at oblique wave normal angles to the background magnetic field. We find that electromagnetic energy of waves at frequencies below half the electron cyclotron frequency can flow nearly parallel to the ambient magnetic field. We thereby confirm that the gyroaveraging method, which averages the cyclotron motion to the gyrocenter and reduces the simulation from two-dimensional to one-dimensional, is valid for oblique wave-particle interaction. Multiple resonances appear for oblique propagation but not for parallel propagation. We calculate the possible range of resonances with the first-order resonance condition as a function of electron kinetic energy and equatorial pitch angle. To reveal the physical process and the efficiency of electron acceleration by multiple resonances, we assume a simple uniform wave model with constant amplitude and frequency in space and time. We perform test particle simulations with electrons starting at specific equatorial pitch angles and kinetic energies. The simulation results show that multiple resonances contribute to acceleration and pitch angle scattering of energetic electrons. Especially, we find that electrons with energies of a few hundred keV can be accelerated efficiently to a few MeV through the n = 0 Landau resonance.

リンク情報
DOI
https://doi.org/10.1002/2017RS006245
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000415373900005&DestApp=WOS_CPL
URL
http://orcid.org/0000-0002-6683-3940
ID情報
  • DOI : 10.1002/2017RS006245
  • ISSN : 0048-6604
  • eISSN : 1944-799X
  • ORCIDのPut Code : 36643701
  • Web of Science ID : WOS:000415373900005

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