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A waveguide model of the return stroke channel with a “metamaterial” corona
Author(s) -
Lehtinen Nikolai G.
Publication year - 2012
Publication title -
radio science
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.371
H-Index - 84
eISSN - 1944-799X
pISSN - 0048-6604
DOI - 10.1029/2011rs004749
Subject(s) - physics , optics , wavefront , metamaterial , waveguide , corona (planetary geology) , mechanics , computational physics , materials science , astrobiology , venus
We model the lightning return stroke channel as a three layer cylindrical waveguide, consisting of (1) highly conducting thin core channel; (2) “metamaterial” corona, i.e., corona with an effective bulk anisotropic dielectric permittivity tensor which is due to the fine structure of leaders branching away from the main channel; and (3) the surrounding non‐conducting air. The lowest axially symmetric TM mode in this waveguide represents the return stroke current wave. We find time‐ and space‐domain solutions for the current wave in a channel connected to the ground driven by an axial current of Bruce‐Golde model temporal shape concentrated at the point of the channel connection to the ground. The front of the current wave is found to be dispersed, and the speed of the front is significantly (by a factor of 5–10 for some parameters) slower than the speed of light. The calculated radial electric field is found to be consistent with experimental measurements. When the second layer of the waveguide is filled with an isotropic material, the slowdown of the wavefront is found to be smaller. The time‐ and space‐domain calculations are also supported by the numerical solution of a dispersion equation, which shows that the phase velocity may be significantly less than the speed of light.