2006
DOI: 10.1016/j.asr.2005.01.073
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Influence of ionospheric conductivity on the ballooning modes in the inner magnetosphere of the Earth

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Cited by 27 publications
(20 citation statements)
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“…This statement is additionally proven by this article, as it shows that in the case of curved magnetic field lines, the transversal amplitude of flute perturbations deviates from the constant and is accompanied by significant longitudinal displacements. The stability criterion derived in the paper by Cheremnykh and Parnowski (2006a) and later improved in the paper by Cheremnykh and Parnowski (2006b) is by about one-third less than the Gold criterion (∼4.25 against ∼6.67). Given the problem that radial pressure gradients in the magnetosphere (Lui and Hamilton, 1992;DeMichelis et al, 1999) are insufficient to break the Gold criterion, it is crucial to determine which instabilities can be triggered in the magnetosphere.…”
Section: Introductionmentioning
confidence: 96%
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“…This statement is additionally proven by this article, as it shows that in the case of curved magnetic field lines, the transversal amplitude of flute perturbations deviates from the constant and is accompanied by significant longitudinal displacements. The stability criterion derived in the paper by Cheremnykh and Parnowski (2006a) and later improved in the paper by Cheremnykh and Parnowski (2006b) is by about one-third less than the Gold criterion (∼4.25 against ∼6.67). Given the problem that radial pressure gradients in the magnetosphere (Lui and Hamilton, 1992;DeMichelis et al, 1999) are insufficient to break the Gold criterion, it is crucial to determine which instabilities can be triggered in the magnetosphere.…”
Section: Introductionmentioning
confidence: 96%
“…Then we cast the dipole magnetic field into them and rewrite them for an individual magnetic field line, taking into account that ballooning perturbations are fieldline-driven. After that, we rewrote them in a dimensionless form (Cheremnykh and Parnowski, 2006b) 2 c 6 b …”
Section: The Equations Of Small Oscillationsmentioning
confidence: 99%
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“…Therefore, influence of the ionospheric boundaries on the ballooning mode properties can be neglected, assuming that the growing disturbances are localized in the near-equatorial region of the nightside magnetosphere. The influence of the ionospheric boundary conditions on the ballooning modes was considered in many papers (e.g., Cheremnykh and Parnowski, 2006). 2.1 Asymptotic theory of transverse small-scale disturbances For small-scale in the transverse (across B) direction disturbances the linearized MHD equations of a finite pressure plasma can be simplified and reduced to a system of ordinary differential equations for coupled Alfven and SMS modes.…”
Section: Mhd Plasma Equilibrium and Linearized Dynamic Equationsmentioning
confidence: 99%