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Open AccessJournal ArticleDOI

Effects of ionospheric scintillation on Transit satellite measurement of total electron content

D. L. Knepp
- 01 Feb 2004 - 
- Vol. 39, Iss: 1
TLDR
In this article, a numerical phase screen propagation simulation is applied to study the accuracy of the measurement of total electron content (TEC) made with Transit-like signals, where the phase from coherently related 150 and 400 MHz tones is combined to obtain an estimate of the phase imparted to a propagating signal by transmission through the ionosphere.
Abstract
[1] Ionospheric scintillation can affect not only satellite communications but also satellite measurements of the ionosphere, such as the measurements of total electron content (TEC) made using Transit-like signal transmissions. In this work a numerical phase-screen propagation simulation is applied to study the accuracy of the measurement of TEC made with Transit-like signals. To measure TEC, the phase from coherently related 150 and 400 MHz tones is combined to obtain an estimate of the phase imparted to a propagating signal by transmission through the ionosphere. This phase is processed to remove ambiguities of 2π and converted to a relative value of TEC. However, scattering caused by ionospheric irregularities produces amplitude fading and phase variations that degrade the TEC measurement in several ways. Rapid phase variations that may be associated with deep fades can degrade the phase-ambiguity removal process. Fresnel filtering causes scintillation when intrinsic ionospheric variations are of the size of the Fresnel zone and smaller. Receiver noise also acts to degrade the phase measurements and is especially important during the deepest fades. This paper considers the effects of all these processes and develops rule-of-thumb qualifiers to assure the accuracy of Transit-like measurements of TEC.

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Citations
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Journal ArticleDOI

Variability of ionospheric scintillation near the equatorial anomaly crest of the Indian zone

TL;DR: In this article, multistation observations of ionosphere scintillation at VHF (250 MHz) and GNSS L1 frequency from three locations at ~ 1° latitudinal separations near the northern crest of the equatorial ionization anomaly (EIA) of the Indian longitude sector were investigated in conjunction with total electron content (TEC) data and available ionosonde data near the magnetic equator.
Journal ArticleDOI

Comparison of 4 methods for transionospheric scintillation evaluation

TL;DR: In this article, a comparison is made between four different methods of scintillation determination (the phase screen method, the Hybrid method, geometrical optics and the Rytov method) for transionospheric paths at GNSS frequencies.
Journal ArticleDOI

The effect of phase scintillations on the accuracy of phase screen simulation using deterministic screens derived from GPS and ALTAIR measurements

TL;DR: In this article, the effect of phase scintillations on the accuracy of phase screen simulation when using the phase measured on the ground as a proxy for the ionospheric screen was investigated.
Journal ArticleDOI

Stochastic TEC Structure Characterization

TL;DR: In this article, the authors show that the phase-scintillation errors are a negligibly small fraction of the stochastic TEC component for most global navigation satellite system operating conditions.
Journal ArticleDOI

A comparative study between two percentage of occurrence methodologies for computing ionospheric scintillation statistics

TL;DR: A detailed comparative analysis of the two widely used percentage of occurrence methodologies used to compute the statistics of ionospheric scintillation activity based on the data of a Global Positioning System (GPS) Ionospheric Scintillation and (TEC) Total Electron Content Monitor (GISTM) receiver located at the northern Equatorial Ionization Anomaly (EIA) crest region Agartala (23.76°N, 91.26°E) of the Indian subcontinent, during 2012-2015 of the rising, peak and declining solar activity
References
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Journal ArticleDOI

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TL;DR: An extended random medium is modeled by a set of 2-D thin Gaussian phase-changing screens with phase power spectral densities appropriate to the natural medium being modeled, showing that under weak scattering the small-scale Fresnel length structure of the medium dominates the intensity scattering pattern.
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Journal ArticleDOI

Multiple phase-screen calculation of the temporal behavior of stochastic waves

D.L. Knepp
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Journal ArticleDOI

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TL;DR: In this paper, the authors reviewed the opportunities to use the Global Positioning System (GPS) for ionospheric total electron content (TEC) research and showed that with appropriate smoothing, GPS TECs can be used to extend the existing database.
Journal ArticleDOI

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TL;DR: In this article, the authors used the Wideband ionospheric scintillation model (WBMOD) to calculate the S 4 on a two-way channel, where the data from three additional stations (Ascension Island, in the South Atlantic Ocean, Huancayo, Peru, and Manila, Phillipines; data collected under the auspices of the USAF Phillips Laboratory Geophysics Directorate) were used to provide a greater diversity in both latitude and longitude.
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