scholarly journals The Acceleration of Electrons to High Energies Over the Jovian Polar Cap via Whistler Mode Wave-Particle Interactions

2018 ◽  
Vol 123 (9) ◽  
pp. 7523-7533 ◽  
Author(s):  
S. S. Elliott ◽  
D. A. Gurnett ◽  
W. S. Kurth ◽  
B. H. Mauk ◽  
R. W. Ebert ◽  
...  
Keyword(s):  
Particle Interactions ◽  
Polar Cap ◽  
Whistler Mode ◽  
Mode Wave ◽  
High Energies ◽  
Whistler Mode Wave ◽  
Wave Particle Interactions

Energetic electron precipitation via oblique whistler mode chorus emissions in the outer radiation belt

2021 ◽  
Author(s):  
Yikai Hsieh ◽  
Yoshiharu Omura
Keyword(s):  
Cyclotron Resonance ◽  
Energetic Electron ◽  
Particle Simulation ◽  
Electron Precipitation ◽  
Particle Interactions ◽  
Outer Radiation Belt ◽  
Whistler Mode ◽  
Mode Wave ◽  
Whistler Mode Wave ◽  
Wave Particle Interactions

<p>Whistler mode chorus emissions in the Earth’s magnetosphere cause energetic electron precipitation and the associated pulsating aurora. First-order cyclotron resonance in parallel whistler mode wave-particle interactions is the main mechanism of the precipitation. Not only cyclotron resonance but also Landau resonance and higher-order cyclotron resonances occur in the oblique whistler mode wave-particle interactions. Especially, electrons can be accelerated and scattered to lower equatorial pitch angles rapidly via Landau resonance. We apply test particle simulation and the Green’s function method to check the energetic electron precipitation caused by oblique chorus emissions. We simulate the wave-particle interactions around L=4.5 for electron ranges from 10 keV to a few MeV. We further compare the precipitation fluxes between parallel and oblique chorus emissions. Our simulation result reveals that oblique chorus emissions lead to more electron precipitation than parallel chorus emissions. At kinetic energy E < 100 keV, the electron precipitation ratio (oblique case/parallel case) is about 1.3. At 100 keV < E < 0.5 MeV, the ratio is greater than 2. At E > 0.5 MeV, the ratio is greater than 2 orders. Multiple resonances effect in the oblique whistler mode wave-particle interactions is the reason for the greater precipitation.</p>

Magnetic field pulses produced via whistler mode wave decay in the ionosphere

1997 ◽  
Vol 4 (12) ◽  
pp. 4388-4393 ◽  
Author(s):  
Vyacheslav Yukhimuk ◽  
Robert Roussel-Dupre
Keyword(s):  
Magnetic Field ◽  
Whistler Mode ◽  
Mode Wave ◽  
Wave Decay ◽  
Whistler Mode Wave

scholarly journals Poloidal Mode Wave-Particle Interactions Inferred From Van Allen Probes and CARISMA Ground-Based Observations

2018 ◽  
Vol 123 (6) ◽  
pp. 4652-4667 ◽  
Author(s):  
C. Wang ◽  
R. Rankin ◽  
Y. Wang ◽  
Q.-G. Zong ◽  
X. Zhou ◽  
...  
Keyword(s):  
Particle Interactions ◽  
Mode Wave ◽  
Van Allen Probes ◽  
Wave Particle Interactions

scholarly journals Whistler mode wave coupling effects on electron dynamics in the near Earth magnetosphere

1998 ◽  
Vol 25 (3) ◽  
pp. 265-268 ◽  
Author(s):  
S. K. Matsoukis ◽  
S. Chapman ◽  
G. Rowlands
Keyword(s):  
Electron Dynamics ◽  
Coupling Effects ◽  
Wave Coupling ◽  
Whistler Mode ◽  
Mode Wave ◽  
Whistler Mode Wave

Whistler-mode wave generation around interplanetary shocks in and out of the ecliptic plane

1995 ◽  
Vol 22 (23) ◽  
pp. 3425-3428 ◽  
Author(s):  
F. Pierre ◽  
J. Solomon ◽  
N. Cornilleau-Wehrlin ◽  
P. Canu ◽  
E. E. Scime ◽  
...  
Keyword(s):  
Ecliptic Plane ◽  
Wave Generation ◽  
Interplanetary Shocks ◽  
Whistler Mode ◽  
Mode Wave ◽  
Whistler Mode Wave
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