VII. Plasma Effects

John W Armstrong

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NASA NTRS · 19830028037

VII. Plasma Effects

John W Armstrong

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Abstract

Radio communication with space probes requires sending signals through the Earth's ionosphere and usually the solar wind. During planetary flybys, the signal may also pass through the ionosphere of another planet. These ionized media can perturb the radio signal in a variety of ways. Examples of these perturbations are variations in the electrical length between the spacecraft and the ground station, Faraday rotation of linearly polarized signals, amplitude and phase scintillations, and spectral and angular broadening. These plasma effects can have undesirable influences on telemetry performance and thus need to be understood from a communications engineering viewpoint. The plasma effects are, however, useful from a scientific viewpoint, since the effects on the communications link can often be inverted to estimate the physical conditions in the plasma.

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BibTeX RIS

John W Armstrong. 1983-07-15. VII. Plasma Effects. https://ntrs.nasa.gov/citations/19830028037

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