Magnetic field influence on aurorae and the Jovian plasma disk radial structure

Autor: E. S. Belenkaya, P. A. Bespalov, S. S. Davydenko, V. V. Kalegaev

Publikováno v: Annales Geophysicae, Vol 24, Pp 973-988 (2006)

The Jovian paraboloid magnetospheric model is applied for the investigation of the planet's auroral emission and plasma disk structure in the middle magnetosphere. Jupiter's auroral emission demonstrates the electrodynamic coupling between the ion

Externí odkaz: https://doaj.org/article/ec516aeea72649f7a7f8476ed8752dfe

Advanced numerical model of lightning development: Application to studying the role of LPCR in determining lightning type

Autor: Artem Syssoev, F. D. Iudin, S. S. Davydenko, D. I. Iudin, E. A. Mareev, Vladimir A. Rakov

Publikováno v: Journal of Geophysical Research: Atmospheres. 122:6416-6430

An advanced 3D numerical model of lightning development is presented. The key features of the model include the probabilistic branching, bidirectional propagation, non-zero internal electric field, simultaneous growth of multiple branches, physical t

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::a116848678eab50f3b892dbad8d2aaec
https://doi.org/10.1002/2016jd026261

Fractal Model of a Compact Intracloud Discharge. I. Features of the Structure and Evolution

Autor: S. S. Davydenko, D. I. Iudin

Publikováno v: Radiophysics and Quantum Electronics. 58:477-496

We propose a new model of a compact intracloud discharge considered as the result of interaction between two (or more) bipolar streamer structures formed in a strong large-scale electric field of a thundercloud. The model assumes two stages of the co

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::8da21d6976c28c6b9aea2b99d334f4df
https://doi.org/10.1007/s11141-015-9621-2

Influence of ionospheric flows on the effect of the planetary electric generator

Autor: S. S. Davydenko

Publikováno v: Geomagnetism and Aeronomy. 52:211-221

Exact distributions of the electric field and current density in the vicinity of the rotating magnetized planet are determined within the planetary electric generator model. The model planetary plasma envelope is assumed to be inhomogeneous and consi

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::f3648de80869f484231521245cc3521a
https://doi.org/10.1134/s0016793212010033

Magnetic field influence on aurorae and the Jovian plasma disk radial structure

Autor: S. S. Davydenko, Elena Belenkaya, P. A. Bespalov, Vladimir Kalegaev

Publikováno v: Annales Geophysicae, Vol 24, Pp 973-988 (2006)
Annales Geophysicae, Vol 24, Iss 3, Pp 973-988 (2006)
Annales Geophysicae
Annales Geophysicae, European Geosciences Union, 2006, 24 (3), pp.973-988

The Jovian paraboloid magnetospheric model is applied for the investigation of the planet's auroral emission and plasma disk structure in the middle magnetosphere. Jupiter's auroral emission demonstrates the electrodynamic coupling between the ionosp

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::067de78994c3df32b488d6529e4fff3d
https://doi.org/10.5194/angeo-24-973-2006