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Cited by 462

The DOI matches its Crossref record; 11 of the 11 references it cites were found in a registry or an index.

A power law phase screen model for ionospheric scintillation: 1. Weak scatter

Rino, C. L.·1979·Radio Science

Abstract

In this paper the weak scatter scintillation theory is reformulated to show explicitly the ramifications of an arbitrarily large ionospheric outer scale. The measured temporal phase spectrum, for example, is effectively truncated at a fixed frequency corresponding to the detrend time or the length of the data interval over which it is measured (whichever is smaller). As a consequence, the rms phase exhibits a complicated dependence on the relative irregularity drift velocity and the propagation geometry. This effect has not been included in previous analyses. By comparison, intensity scintillation data are intrinsically high‐pass filtered by the diffraction process. By taking advantage of this fact a simple closed form expression for the S4 intensity scintillation index has been derived. The theory is applied to representative data sets from the Wideband satellite. The interpretation of the ionospheric parameters deduced from the analysis is also discussed.

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Metadata

Authors
Rino, C. L.
Venue
Radio Science
Published
1979-11
Volume
14
Issue
6
Pages
1135-1145
ISSN
  • 0048-6604 (ISSN-L)
  • 1944-799X
OpenAlex
W2024714333
Cited by
462
References
11
FWCI
19.57
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: A power law phase screen model for ionospheric scintillation: 1. Weak scatter. https://app.cochat.ai/papers/10.1029/rs014i006p01135
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Rino, C. L. (1979). A power law phase screen model for ionospheric scintillation: 1. Weak scatter. Radio Science. https://doi.org/10.1029/rs014i006p01135

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