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Title: Generation of Highly Oblique Lower Band Chorus Via Nonlinear Three-Wave Resonance

Abstract

Chorus in the inner magnetosphere has been observed frequently at geomagnetically active times, typically exhibiting a two-band structure with a quasi-parallel lower band and an upper band with a broad range of wave normal angles. But recent observations by Van Allen Probes confirm another type of lower band chorus, which has a large wave normal angle close to the resonance cone angle. It has been proposed that these waves could be generated by a low-energy beam-like electron component or by temperature anisotropy of keV electrons in the presence of a low-energy plateau-like electron component. This paper, however, presents an alternative mechanism for generation of this highly oblique lower band chorus. Through a nonlinear three-wave resonance, a quasi-parallel lower band chorus wave can interact with a mildly oblique upper band chorus wave, producing a highly oblique quasi-electrostatic lower band chorus wave. This theoretical analysis is confirmed by 2-D electromagnetic particle-in-cell simulations. Furthermore, as the newly generated waves propagate away from the equator, their wave normal angle can further increase and they are able to scatter low-energy electrons to form a plateau-like structure in the parallel velocity distribution. As a result, the three-wave resonance mechanism may also explain the generation of quasi-parallelmore » upper band chorus which has also been observed in the magnetosphere.« less

Authors:
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3]; ORCiD logo [4]; ORCiD logo [4]
  1. New Mexico Consortium, Los Alamos, NM (United States)
  2. Space Science Institute, Boulder, CO (United States)
  3. New Mexico Consortium, Los Alamos, NM (United States); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  4. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Publication Date:
Research Org.:
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Sponsoring Org.:
National Aeronautic and Space Administration (NASA); USDOE
OSTI Identifier:
1415428
Report Number(s):
LA-UR-17-30358
Journal ID: ISSN 0094-8276; TRN: US1800821
Grant/Contract Number:  
AC52-06NA25396
Resource Type:
Accepted Manuscript
Journal Name:
Geophysical Research Letters
Additional Journal Information:
Journal Volume: 44; Journal Issue: 19; Journal ID: ISSN 0094-8276
Publisher:
American Geophysical Union
Country of Publication:
United States
Language:
English
Subject:
58 GEOSCIENCES; Heliospheric and Magnetospheric Physics; oblique whistler; three-wave resonance; PIC simulation; ray tracing

Citation Formats

Fu, Xiangrong, Gary, Stephen Peter, Reeves, Geoffrey D., Winske, Dan, and Woodroffe, Jesse Richard. Generation of Highly Oblique Lower Band Chorus Via Nonlinear Three-Wave Resonance. United States: N. p., 2017. Web. doi:10.1002/2017GL074411.
Fu, Xiangrong, Gary, Stephen Peter, Reeves, Geoffrey D., Winske, Dan, & Woodroffe, Jesse Richard. Generation of Highly Oblique Lower Band Chorus Via Nonlinear Three-Wave Resonance. United States. doi:10.1002/2017GL074411.
Fu, Xiangrong, Gary, Stephen Peter, Reeves, Geoffrey D., Winske, Dan, and Woodroffe, Jesse Richard. Tue . "Generation of Highly Oblique Lower Band Chorus Via Nonlinear Three-Wave Resonance". United States. doi:10.1002/2017GL074411. https://www.osti.gov/servlets/purl/1415428.
@article{osti_1415428,
title = {Generation of Highly Oblique Lower Band Chorus Via Nonlinear Three-Wave Resonance},
author = {Fu, Xiangrong and Gary, Stephen Peter and Reeves, Geoffrey D. and Winske, Dan and Woodroffe, Jesse Richard},
abstractNote = {Chorus in the inner magnetosphere has been observed frequently at geomagnetically active times, typically exhibiting a two-band structure with a quasi-parallel lower band and an upper band with a broad range of wave normal angles. But recent observations by Van Allen Probes confirm another type of lower band chorus, which has a large wave normal angle close to the resonance cone angle. It has been proposed that these waves could be generated by a low-energy beam-like electron component or by temperature anisotropy of keV electrons in the presence of a low-energy plateau-like electron component. This paper, however, presents an alternative mechanism for generation of this highly oblique lower band chorus. Through a nonlinear three-wave resonance, a quasi-parallel lower band chorus wave can interact with a mildly oblique upper band chorus wave, producing a highly oblique quasi-electrostatic lower band chorus wave. This theoretical analysis is confirmed by 2-D electromagnetic particle-in-cell simulations. Furthermore, as the newly generated waves propagate away from the equator, their wave normal angle can further increase and they are able to scatter low-energy electrons to form a plateau-like structure in the parallel velocity distribution. As a result, the three-wave resonance mechanism may also explain the generation of quasi-parallel upper band chorus which has also been observed in the magnetosphere.},
doi = {10.1002/2017GL074411},
journal = {Geophysical Research Letters},
number = 19,
volume = 44,
place = {United States},
year = {2017},
month = {9}
}

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Cited by: 11 works
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Works referenced in this record:

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