✦ LIBER ✦

Nonlinear wave structures in collisional plasma of auroral E-region ionosphere

✍ Scribed by A. V. Volosevich; Yu. I. Galperin

Publisher: Copernicus Group
Year: 1997
Tongue: English
Weight: 297 KB
Volume: 15
Category: Article
ISSN: 0992-7689
DOI: 10.1007/s00585-997-0890-8

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Propagation of lower hybrid resonance wa

Propagation of lower hybrid resonance waves in depleted-plasma regions in the upper auroral ionosphere

✍ D. L. Pasmanik; A. G. Demekhov; V. Yu. Trakhtengerts; E. E. Titova; M. J. Rycrof 📂 Article 📅 2009 🏛 Springer US 🌐 English ⚖ 293 KB

Observations of nightside auroral plasma

Observations of nightside auroral plasma upflows in the F-region and topside ionosphere

✍ C. Foster; M. Lester 📂 Article 📅 1996 🏛 Copernicus Group 🌐 English ⚖ 483 KB

The role of natural E-region plasma turb

The role of natural E-region plasma turbulence in the enhanced absorption of HF radio waves in the auroral ionosphere:Implications for RF heating of the auroral electrojet

✍ T. R. Robinson 📂 Article 📅 1994 🏛 Copernicus Group 🌐 English ⚖ 55 KB

A comment on “nonlinear solitary wave in

A comment on “nonlinear solitary wave in the ionospheric E-region” by Arykov and Maltsev

✍ T.R. Robinson 📂 Article 📅 1997 🏛 Elsevier Science 🌐 English ⚖ 92 KB

On the Nonlinear Theory of Surface Wave

On the Nonlinear Theory of Surface Wave Excitation in a Collisional Solid State Plasma

✍ V. K. Grishin; M. F. Kanevskii; S. T. Ivanov 📂 Article 📅 1984 🏛 John Wiley and Sons 🌐 English ⚖ 328 KB 👁 2 views

The nonlinear equations governing relativistic electron beam-surface wave dynamics in dissipative P-S-plasma are derived. The influence of P-plasma on time saturation, amplitude of the wave at saturation and damping factor is analyzed. The obtained results are discussed from the physical point of vi

Self-organization of planetary electroma

Self-organization of planetary electromagnetic waves in the E-region of the ionosphere

✍ G.D. Aburjania; G.V. Jandieri; A.G. Khantadze 📂 Article 📅 2003 🏛 Elsevier Science 🌐 English ⚖ 250 KB

A physical mechanism for the generation of slow and fast electromagnetic-type planetary waves due to standing factorlatitude variation of geomagnetic ÿeld-in the dissipative E-region of the ionosphere is suggested. It has been shown that slow waves are generated due to the dynamo-ÿeld in the ionosph