Access the full text.
Sign up today, get DeepDyve free for 14 days.
R. Thorne, W. Li, B. Ni, Q. Ma, J. Bortnik, Lunjin Chen, D. Baker, H. Spence, G. Reeves, M. Henderson, C. Kletzing, W. Kurth, G. Hospodarsky, J. Blake, J. Fennell, S. Claudepierre, S. Kanekal (2013)
Rapid local acceleration of relativistic radiation-belt electrons by magnetospheric chorusNature, 504
Wen Li, J. Bortnik, R. Thorne, C. Cully, L. Chen, V. Angelopoulos, Y. Nishimura, J. Tao, J. Bonnell, O. Lecontel (2013)
Characteristics of the Poynting flux and wave normal vectors of whistler‐mode waves observed on THEMISJournal of Geophysical Research: Space Physics, 118
O. Santolík, D. Gurnett, J. Pickett, M. Parrot, N. Cornilleau-Wehrlin (2005)
Central position of the source region of storm-time chorusPlanetary and Space Science, 53
W. Li, R. Thorne, V. Angelopoulos, J. Bortnik, C. Cully, Binbin Ni, O. Lecontel, Alain Roux, U. Auster, W. Magnes (2009)
Global distribution of whistler‐mode chorus waves observed on the THEMIS spacecraftGeophysical Research Letters, 36
R. Thorne, B. Ni, X. Tao, R. Horne, N. Meredith (2010)
Scattering by chorus waves as the dominant cause of diffuse auroral precipitationNature, 467
R. Horne, R. Thorne (1998)
Potential waves for relativistic electron scattering and stochastic acceleration during magnetic stormsGeophysical Research Letters, 25
Xiangrong Fu, M. Cowee, R. Friedel, H. Funsten, S. Gary, G. Hospodarsky, C. Kletzing, W. Kurth, Brian Larsen, Kaijun Liu, Elizabeth MacDonald, K. Min, Geoff Reeves, Ruth Skoug, D. Winske (2014)
Whistler anisotropy instabilities as the source of banded chorus: Van Allen Probes observations and particle-in-cell simulationsJournal of Geophysical Research. Space Physics, 119
R. Helliwell (1967)
A theory of discrete VLF emissions from the magnetosphereJournal of Geophysical Research, 72
Zhou Lu, Gan Zhong-wei, Li Gao-xiang (2004)
Quantum Interference Between Decay Channels of a Three-Level Atom Placed Between Two Parallel PlatesChinese Physics Letters, 21
W. Burtis, R. Helliwell (1969)
Banded chorus - A new type of VLF radiation observed in the magnetosphere by OGO 1 and OGO 3.Journal of Geophysical Research, 74
Xinliang Gao, Q. Lu, Shui Wang (2017)
First report of resonant interactions between whistler mode waves in the Earth's magnetosphereGeophysical Research Letters, 44
F. Mottez (2012)
Non-propagating electric and density structures formed through non-linear interaction of Alfvén wavesAnnales Geophysicae, 30
Y. Omura, Y. Katoh, D. Summers (2008)
Theory and simulation of the generation of whistler‐mode chorusJournal of Geophysical Research, 113
F. Xiao, Chang Yang, Zhaoguo He, Z. Su, Qinghua Zhou, Yihua He, C. Kletzing, W. Kurth, G. Hospodarsky, H. Spence, G. Reeves, H. Funsten, J. Blake, D. Baker, J. Wygant (2014)
Chorus acceleration of radiation belt relativistic electrons during March 2013 geomagnetic stormJournal of Geophysical Research: Space Physics, 119
Lu Quan-Ming, Wang Lian-qi, Zhou Yan, Wang Shui (2004)
Electromagnetic Instabilities Excited by Electron Temperature AnisotropyChinese Physics Letters, 21
W. Li, R. Thorne, J. Bortnik, X. Tao, V. Angelopoulos (2012)
Characteristics of hiss‐like and discrete whistler‐mode emissionsGeophysical Research Letters, 39
W. Li, J. Bortnik, R. Thorne, V. Angelopoulos (2011)
Global distribution of wave amplitudes and wave normal angles of chorus waves using THEMIS wave observationsJournal of Geophysical Research, 116
Xiangrong Fu, S. Gary, G. Reeves, D. Winske, J. Woodroffe (2017)
Generation of Highly Oblique Lower Band Chorus Via Nonlinear Three‐Wave ResonanceGeophysical Research Letters, 44
R. Horne, R. Thorne, N. Meredith, R. Anderson (2003)
Diffuse auroral electron scattering by electron cyclotron harmonic and whistler mode waves during an isolated substormJournal of Geophysical Research, 108
J. Scharer, A. Trivelpiece (1967)
Cyclotron Wave Instabilities in a PlasmaPhysics of Fluids, 10
Xinliang Gao, D. Mourenas, Wen Li, A. Artemyev, Q. Lu, X. Tao, Shui Wang (2016)
Observational evidence of generation mechanisms for very oblique lower band chorus using THEMIS waveform dataJournal of Geophysical Research: Space Physics, 121
B. Ni, R. Thorne, N. Meredith, Y. Shprits, R. Horne (2011)
Diffuse auroral scattering by whistler mode chorus waves: Dependence on wave normal angle distributionJournal of Geophysical Research, 116
M. LeDocq, D. Gurnett, G. Hospodarsky (1998)
Chorus source locations from VLF Poynting flux measurements with the Polar spacecraftGeophysical Research Letters, 25
T. Terasawa, M. Hoshino, J. Sakai, T. Hada (1986)
Decay instability of finite-amplitude circularly polarized Alfven waves - A numerical simulation of stimulated Brillouin scatteringJournal of Geophysical Research, 91
S. Gary, D. Winske, M. Hesse (2000)
Electron temperature anisotropy instabilities: Computer simulationsJournal of Geophysical Research, 105
Xinliang Gao, Q. Lu, J. Bortnik, Wen Li, Lunjin Chen, Shui Wang (2016)
Generation of multiband chorus by lower band cascade in the Earth's magnetosphereGeophysical Research Letters, 43
S. Gary, H. Karimabadi (2006)
Linear theory of electron temperature anisotropy instabilities: Whistler, mirror, and WeibelJournal of Geophysical Research, 111
D. Summers, R. Thorne, F. Xiao (1998)
Relativistic theory of wave‐particle resonant diffusion with application to electron acceleration in the magnetosphereJournal of Geophysical Research, 103
B. Tsurutani, E. Smith (1974)
Postmidnight chorus: A substorm phenomenonJournal of Geophysical Research, 79
X. Gao, W. Li, R. Thorne, J. Bortnik, V. Angelopoulos, Q. Lu, X. Tao, S. Wang (2014)
Statistical results describing the bandwidth and coherence coefficient of whistler mode waves using THEMIS waveform dataJournal of Geophysical Research: Space Physics, 119
W. Li, R. Thorne, Y. Nishimura, J. Bortnik, V. Angelopoulos, J. Mcfadden, D. Larson, J. Bonnell, O. Contel, A. Roux, U. Auster (2010)
THEMIS analysis of observed equatorial electron distributions responsible for the chorus excitationJournal of Geophysical Research, 115
N. Meredith, R. Horne, R. Anderson (2001)
Substorm dependence of chorus amplitudes: Implications for the acceleration of electrons to relativistic energiesJournal of Geophysical Research, 106
B. Ni, R. Thorne, Y. Shprits, J. Bortnik (2008)
Resonant scattering of plasma sheet electrons by whistler‐mode chorus: Contribution to diffuse auroral precipitationGeophysical Research Letters, 35
A. Craik (1986)
Three-wave resonance
R. Sydora, K. Sauer, I. Silin (2007)
Coherent whistler waves and oscilliton formation: Kinetic simulationsGeophysical Research Letters, 34
B. Milligen, E. Sánchez, T. Estrada, C. Hidalgo, B. Brañas, B. Carreras, L. García (1995)
Wavelet bicoherence: A new turbulence analysis toolPhysics of Plasmas, 2
Huayue Chen, Xinliang Gao, Q. Lu, Yangguang Ke, Shui Wang (2017)
Lower Band Cascade of Whistler Waves Excited by Anisotropic Hot Electrons: One‐Dimensional PIC SimulationsJournal of Geophysical Research: Space Physics, 122
R. Burton, R. Holzer (1974)
The origin and propagation of chorus in the outer magnetosphereJournal of Geophysical Research, 79
Jun Guo (2016)
The generation and evolution of multi-band EMIC waves in the magnetosphere: Hybrid simulationsAdvances in Space Research, 58
Q. Lu, Lihui Zhou, Shui Wang (2010)
Particle‐in‐cell simulations of whistler waves excited by an electron κ distribution in space plasmaJournal of Geophysical Research, 115
M. Parrot, O. Santolík, N. Cornilleau-Wehrlin, M. Maksimović, C. Harvey (2003)
Source location of chorus emissions observed by ClusterAnnales Geophysicae, 21
Xinliang Gao, Wen Li, R. Thorne, J. Bortnik, V. Angelopoulos, Q. Lu, X. Tao, Shui Wang (2014)
New evidence for generation mechanisms of discrete and hiss‐like whistler mode wavesGeophysical Research Letters, 41
Yangguang Ke, Xinliang Gao, Q. Lu, Xueyi Wang, Shui Wang (2017)
Generation of rising‐tone chorus in a two‐dimensional mirror field by using the general curvilinear PIC codeJournal of Geophysical Research: Space Physics, 122
Xinliang Gao, Yangguang Ke, Q. Lu, Lunjin Chen, Shui Wang (2017)
Generation of Multiband Chorus in the Earth's Magnetosphere: 1‐D PIC SimulationGeophysical Research Letters, 44
C. Kennel, H. Petschek (1966)
LIMIT ON STABLY TRAPPED PARTICLE FLUXESJournal of Geophysical Research, 71
Y. Nishimura, J. Bortnik, W. Li, R. Thorne, B. Ni, L. Lyons, V. Angelopoulos, Y. Ebihara, J. Bonnell, O. Contel, U. Auster (2013)
Structures of dayside whistler‐mode waves deduced from conjugate diffuse auroraJournal of Geophysical Research: Space Physics, 118
O. Santolík, D. Gurnett, J. Pickett, M. Parrot, N. Cornilleau-Wehrlin (2003)
Spatio-temporal structure of storm-time chorusJournal of Geophysical Research, 108
K. Lorentzen, J. Blake, U. Inan, J. Bortnik (2001)
Observations of relativistic electron microbursts in association with VLF chorusJournal of Geophysical Research, 106
Li (2010)
A00F11Journal of Geophysical Research, 115
J. Burch, T. Moore, R. Torbert, B. Giles (2016)
Magnetospheric Multiscale Overview and Science ObjectivesSpace Science Reviews, 199
Nonlinear physical processes related to whistler mode waves are attracting more and more attention for their significant role in reshaping whistler mode spectra in the Earth's magnetosphere. Using a 1‐D particle‐in‐cell simulation model, we have investigated the nonlinear evolution of parallel counter‐propagating whistler mode waves excited by anisotropic electrons within the equatorial source region. In our simulations, after the linear phase of whistler mode instability, the strong electrostatic standing structures along the background magnetic field will be formed, resulting from the coupling between excited counter‐propagating whistler mode waves. The wave numbers of electrostatic standing structures are about twice those of whistler mode waves generated by anisotropic hot electrons. Moreover, these electrostatic standing structures can further be coupled with either parallel or antiparallel propagating whistler mode waves to excite high‐k modes in this plasma system. Compared with excited whistler mode waves, these high‐k modes typically have 3 times wave number, same frequency, and about 2 orders of magnitude smaller amplitude. Our study may provide a fresh view on the evolution of whistler mode waves within their equatorial source regions in the Earth's magnetosphere.
Journal of Geophysical Research: Space Physics – Wiley
Published: Jan 1, 2018
Keywords: ; ; ; ; ;
Read and print from thousands of top scholarly journals.
Already have an account? Log in
Bookmark this article. You can see your Bookmarks on your DeepDyve Library.
To save an article, log in first, or sign up for a DeepDyve account if you don’t already have one.
Copy and paste the desired citation format or use the link below to download a file formatted for EndNote
Access the full text.
Sign up today, get DeepDyve free for 14 days.
All DeepDyve websites use cookies to improve your online experience. They were placed on your computer when you launched this website. You can change your cookie settings through your browser.