scholarly journals Ray trajectories of lower hybrid solitary structures

Author(s):  
P. W. Schuck ◽  
J. W. Bonnell
1978 ◽  
Vol 21 (12) ◽  
pp. 2263 ◽  
Author(s):  
Jean-Marie Wersinger ◽  
Edward Ott ◽  
John M. Finn

2003 ◽  
Vol 31 (6) ◽  
pp. 1125-1177 ◽  
Author(s):  
P.W. Schuck ◽  
J.W. Bonnell ◽  
P.M. Kintner

1998 ◽  
Vol 103 (A4) ◽  
pp. 6935-6953 ◽  
Author(s):  
P. W. Schuck ◽  
C. E. Seyler ◽  
J.-L. Pinçon ◽  
J. W. Bonnell ◽  
P. M. Kintner

1997 ◽  
Vol 102 (A8) ◽  
pp. 17283-17296 ◽  
Author(s):  
J. L. Pinçon ◽  
P. M. Kintner ◽  
P. W. Schuck ◽  
C. E. Seyler

2009 ◽  
Vol 27 (3) ◽  
pp. 1027-1033 ◽  
Author(s):  
J. O. Hall ◽  
G. Stenberg ◽  
A. I. Eriksson ◽  
M. André

Abstract. We investigate the possibility that lower-hybrid solitary structures (LHSS), which are frequently observed in the Earth's ionosphere and magnetosphere, are formed as a result of a modulational interaction between lower-hybrid and dispersive Alfvén waves of initially small amplitude. A large amplitude lower-hybrid pump wave can excite density structures with length scales transverse to the geomagnetic field of the order of the ion gyroradius via a modulational instability. The structure formation in the nonlinear stage of the instability is investigated by numerical solutions of the governing equations, using plasma parameters relevant for LHSS observations in the upper ionosphere and in the magnetosphere. The numerical solutions reveal that the lower-hybrid waves become self-localized inside cylindrically symmetric (with respect to the ambient magnetic field) density cavities, in qualitative agreement with observations. Our model includes thermal electron effects but shows no stabilization at the ion sound gyroradius, suggesting that any preference of observed LHSS for that perpendicular scale likely is due to processes arresting the cavity collapse.


2007 ◽  
Vol 14 (8) ◽  
pp. 082901 ◽  
Author(s):  
D. Jovanović ◽  
P. K. Shukla ◽  
G. Morfill

2002 ◽  
Vol 67 (2-3) ◽  
pp. 149-161 ◽  
Author(s):  
B. V. LUNDIN ◽  
C. KRAFFT

A modified electron whistler dispersion law is derived in the cold-plasma approximation for analytical treatment and simplified numerical calculations of wave propagation in a wide range of ratios ωc/ωp of electron gyro- to plasma frequencies if the wave frequency is much less than ωp. The net contribution of ions to the wave dispersion law is expressed through the value of the lower-hybrid resonance frequency ωlhr only. This approximate dispersion law is valid in a wide frequency domain, that is, from the range of ωlhr until the domain where the contribution of ions can be neglected. A comparison of geometrical-optics ray trajectories calculated by the use of modified and total cold-plasma electron whistler dispersion laws is presented for the case of the Earth's plasma environment. Computer simulations of dynamical spectra of whistler waves excited by lightning discharges and registered in remote regions of the Earth's plasmasphere reveal good numerical stability of the developed ray-tracing code.


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