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Ionospheric scintillation

R.K. Crane
TLDR
In this article, available observations of ionospheric scintillation are analyzed to evaluate the adequacy of existing models used for the interpretation of scintillant data. And the authors used the models were used to construct Scintillation occurrence distribution functions.
Abstract
Available observations of ionospheric scintillation are analyzed to evaluate the adequacy of existing models used for the interpretation of scintillation data. The theoretical models are reviewed and the frequency and propagation geometry dependences predicted by the models are compared with the observations. The models were used to construct scintillation occurrence distribution functions which show that scintillation phenomena significantly affect the design of transionospheric radar or communication systems operating at frequencies below 1 GHz. Diversity schemes useful for mitigation of scintillation effects are considered. Mention is made of the geophysical processes thought to be responsible for scintillation.

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Citations
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Journal ArticleDOI

Radio wave scintillations in the ionosphere

TL;DR: In this article, a review of scintillation of radio waves propagating through the ionosphere is presented, focusing on propagational aspects, including both theoretical and experimental results, with a discussion of the motivation for stochastic formulation of the problem.
Journal ArticleDOI

Global morphology of ionospheric scintillations

TL;DR: In this article, a review of the available amplitude and phase scintillation data is presented, where the effect of magnetic activity, solar sunspot cycle, and time of day is shown for each three latitudinal sectors.
Journal ArticleDOI

A power law phase screen model for ionospheric scintillation: 2. Strong scatter

C. L. Rino
- 01 Nov 1979 - 
TL;DR: In this article, the weak scatter scintillation theory is reformulated to show explicitly the ramifications of an arbitrarily large ionospheric outer scale, which is applied to representative data sets from the Wideband satellite.
Journal ArticleDOI

Tutorial review of synthetic-aperture radar (SAR) with applications to imaging of the ocean surface

TL;DR: In this article, a synthetic aperture radar (SAR) is used to produce high-resolution two-dimensional images of mapped areas, where the amplitude and phase of received signals are collected for the duration of an integration time after which the signal is processed.
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Electromagnetic beam propagation in turbulent media: An update

TL;DR: In this article, the authors reviewed the recent developments on wave propagation in turbulent media, including adaptive optics, intensity scintillations, pulse propagation, atmospheric measurements at visible, IR, and millimeter wave frequencies, speckle interferometry, and other related topics.
References
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A unifying theory of high-latitude geophysical phenomena and geomagnetic storms

TL;DR: In this article, the occurrence at high latitudes of a large number of geophysical phenomena, including geomagnetic agitation and bay disturbances, aurorae, and various irregular distri...
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Coordinates for Mapping the Distribution of Magnetically Trapped Particles

TL;DR: In this article, it is shown that a parameter L = f(B,I) can be defined which retains most of the desirable properties of I and has the additional property of organizing measurements along lines of force.
Journal ArticleDOI

Global morphology of ionospheric scintillations

TL;DR: In this article, a review of the available amplitude and phase scintillation data is presented, where the effect of magnetic activity, solar sunspot cycle, and time of day is shown for each three latitudinal sectors.
Journal ArticleDOI

Electromagnetic beam propagation in turbulent media

R.L. Fante
TL;DR: In this article, the most recent developments on the propagation of optical beams in a turbulent medium, such as the clear atmosphere, are reviewed, including beam spreading, beam wander, loss of coherence, scintillations, angle-of-arrival variations, and short-pulse effects.
Journal ArticleDOI

Polarization fields produced by winds in the equatorial F-region

TL;DR: In this article, the E-layer conductivity may be too small to close this circuit, so that polarization fields build up in the F-layer, causing the plasma to drift with the wind.
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