2019
DOI: 10.1134/s1063780x19070080
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Matrix Algorithm of Approximate Solution of Wave Equations in Inhomogeneous Magnetoactive Plasma

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Cited by 4 publications
(2 citation statements)
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“…where c is the speed of light in free space andε is the permittivity tensor, which yield a set of four equations for the horizontal components E ⊥ (n ⊥ , z), H ⊥ (n ⊥ , z) (in a case of a source-free medium, see, e.g., Budden, 1985, Bespalov et al, 2018, and Mizonova, 2019 dF /dz =MF + Z 0 I δ(z − z s ).…”
Section: Basic Equationsmentioning
confidence: 99%
“…where c is the speed of light in free space andε is the permittivity tensor, which yield a set of four equations for the horizontal components E ⊥ (n ⊥ , z), H ⊥ (n ⊥ , z) (in a case of a source-free medium, see, e.g., Budden, 1985, Bespalov et al, 2018, and Mizonova, 2019 dF /dz =MF + Z 0 I δ(z − z s ).…”
Section: Basic Equationsmentioning
confidence: 99%
“…where c is the speed of light in free space andε is permittivity tensor, which yield a set of four equations for the horizontal components E ⊥ (n ⊥ , z), H ⊥ (n ⊥ , z) (in a case of source-free medium see, e.g., Budden, 1985;Bespalov et al, 2018;Mizonova, 2019)…”
Section: Basic Equationsmentioning
confidence: 99%