1992
DOI: 10.1007/bf00054649
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Absorption of very low frequency (VLF) waves in the whistler mode propagation in Jovian ionosphere

Abstract: Making use of currently available theory of wave absorption, an attempt has been made to estimate the refractive indices and absorption coefficients for different wave frequencies during day and night times in the Jovian ionosphere. The results obtained have striking similarity with the corresponding results in the case of the Earth's ionosphere. It is concluded that VLF signals can be observed more easily during night times.

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Cited by 2 publications
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“…The simultaneous presence of parallel and perpendicular fields will cause the diffusion and modification of whistler mode I I I I I I I I I I energy. Recently Ahmad et al (1992) have carried out theoretically the absorption of very low frequency (VLF) waves in Jovian ionosphere during day and night times. It is concluded with the help of their results that the VLF signals can be more easily observed in the night side of 10 plasma torus resembled those found in earth's plasma-sphere.…”
Section: Formulation Results and Discussionmentioning
confidence: 99%
“…The simultaneous presence of parallel and perpendicular fields will cause the diffusion and modification of whistler mode I I I I I I I I I I energy. Recently Ahmad et al (1992) have carried out theoretically the absorption of very low frequency (VLF) waves in Jovian ionosphere during day and night times. It is concluded with the help of their results that the VLF signals can be more easily observed in the night side of 10 plasma torus resembled those found in earth's plasma-sphere.…”
Section: Formulation Results and Discussionmentioning
confidence: 99%