ELECTRON CYCLOTRON BERNSTEIN WAVES FOR QUASI-PERPENDICULAR AND OBLIQUE PROPAGATION

In this paper, we investigate the electromagnetic electron cyclotron (EMEC) waves in the magnetosphere of Uranus. By using the method of characteristic solution, the expression for dispersion relation is drawn. Following kinetic approach, the growth rate and real frequency of EMEC waves is studied theoretically, considering the injection of cold plasma beam in the Uranian system. The observations made by a space probe launched by NASA, Voyager 2, showed unusual orientation of planet’s spin axis and presence of more particles in high energy tail in Uranian magnetospheric plasma. Therefore, in this paper Kappa distribution is employed instead of usual Maxwellian distribution. The study is extended to the parallel as well as the oblique propagation of EMEC waves with variation in temperature anisotropy, number density of electrons and angle of propagation with respect to magnetic field direction. It is found that these parameters support the growth rate of EMEC waves. But response of real frequency of these waves is not same as that of growth rate for all the cases. Numerical analysis also revealed that as the ratio of number density of cold to hot plasma increases growth rate of EMEC waves also increases. Thus, denser the beam is injected, more the growth can be observed. These results are appropriate for applications to space plasma environments and magnetospheric regimes for detailed comparative planetary study.

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Electron Bernstein waves and narrowband plasma waves near the electron cyclotron frequency in the near-Sun solar wind

Astronomy and Astrophysics ◽

10.1051/0004-6361/202140449 ◽

2021 ◽

Author(s):

D. M. Malaspina ◽

L. B. Wilson III ◽

R. E. Ergun ◽

S. D. Bale ◽

J. W. Bonnell ◽

...

Keyword(s):

Solar Wind ◽

Cyclotron Frequency ◽

Plasma Waves ◽

Electron Cyclotron ◽

Electron Cyclotron Frequency ◽

Bernstein Waves

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Electron-cyclotron maser theory for extraordinary Bernstein waves

Journal of Plasma Physics ◽

10.1017/s0022377897005874 ◽

1997 ◽

Vol 58 (1) ◽

pp. 171-191 ◽

Cited By ~ 15

Author(s):

A. J. WILLES ◽

P. A. ROBINSON

Keyword(s):

Electron Distribution ◽

Electron Cyclotron ◽

Loss Cone ◽

Wave Growth ◽

Electron Cyclotron Maser ◽

Cyclotron Maser ◽

Hybrid Frequency ◽

Bernstein Waves ◽

Bernstein Wave ◽

Cyclotron Harmonic

Electron-cyclotron maser emission is investigated in the regime where wave growth in the electrostatic Bernstein modes dominates (ωp/Ωe>1.5). A semirelativistic growth rate is derived assuming that the wave dispersion is dominated by a cool background electron distribution and the instability is driven by a low-density hot loss-cone-like electron distribution. The properties of Bernstein wave growth are most strongly dependent on the relative temperatures of the hot and cool electron distributions. For Thot/Tcool[gsim ]10, the fastest growing Bernstein waves are produced at frequencies just below each cyclotron harmonic in Bernstein modes lying below the upper-hybrid frequency. For Thot/Tcool[lsim ]10, additional Bernstein modes above the upper-hybrid frequency are excited, with wave frequencies in each excited mode lying significantly above the corresponding cyclotron harmonic. The dependence of Bernstein wave growth on the relative hot and cool electron number densities and emission angle is also discussed.

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Two-stream instabilities from the lower-hybrid frequency to the electron cyclotron frequency: application to the front of quasi-perpendicular shocks

Annales Geophysicae ◽

10.5194/angeo-35-1093-2017 ◽

2017 ◽

Vol 35 (5) ◽

pp. 1093-1112 ◽

Cited By ~ 5

Author(s):

Laurent Muschietti ◽

Bertrand Lembège

Keyword(s):

Shock Front ◽

Cyclotron Frequency ◽

Ion Beam ◽

Wide Frequency Range ◽

Electron Cyclotron ◽

Lower Hybrid ◽

Bernstein Waves ◽

Synthetic View ◽

Drift Instability ◽

The Waves

Abstract. Quasi-perpendicular supercritical shocks are characterized by the presence of a magnetic foot due to the accumulation of a fraction of the incoming ions that is reflected by the shock front. There, three different plasma populations coexist (incoming ion core, reflected ion beam, electrons) and can excite various two-stream instabilities (TSIs) owing to their relative drifts. These instabilities represent local sources of turbulence with a wide frequency range extending from the lower hybrid to the electron cyclotron. Their linear features are analyzed by means of both a dispersion study and numerical PIC simulations. Three main types of TSI and correspondingly excited waves are identified: i. Oblique whistlers due to the (so-called fast) relative drift between reflected ions/electrons; the waves propagate toward upstream away from the shock front at a strongly oblique angle (θ ∼ 50°) to the ambient magnetic field Bo, have frequencies a few times the lower hybrid, and have wavelengths a fraction of the ion inertia length c∕ωpi. ii. Quasi-perpendicular whistlers due to the (so-called slow) relative drift between incoming ions/electrons; the waves propagate toward the shock ramp at an angle θ a few degrees off 90°, have frequencies around the lower hybrid, and have wavelengths several times the electron inertia length c∕ωpe. iii. Extended Bernstein waves which also propagate in the quasi-perpendicular domain, yet are due to the (so-called fast) relative drift between reflected ions/electrons; the instability is an extension of the electron cyclotron drift instability (normally strictly perpendicular and electrostatic) and produces waves with a magnetic component which have frequencies close to the electron cyclotron as well as wavelengths close to the electron gyroradius and which propagate toward upstream. Present results are compared with previous works in order to stress some features not previously analyzed and to define a more synthetic view of these TSIs.

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