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Journal ArticleDOI

Improved amplitude- and phase-scintillation indices derived from wavelet detrended high-latitude GPS data

TLDR
In this article, the performance of a wavelet-based detrending method was evaluated and compared with a new waveletbased detending method using GPS data from high latitudes.
Abstract
Accuracy and validity of scintillation indices estimated using the power and phase of the GPS signal depend heavily on the detrending method used and the selection of the cutoff frequency of the associated filter. A Butterworth filter with a constant cutoff frequency of 0.1 Hz is commonly used in detrending GPS data. In this study, the performance of this commonly used filter is evaluated and compared with a new wavelet-based detrending method using GPS data from high latitudes. It was observed that in detrending high-latitude GPS data, a wavelet filter performed better than Butterworth filters as the correlation between amplitude- and phase-scintillation indices in S 4 and ? ? improved significantly from 0.53, when using a Butterworth filter, to 0.79, when using the wavelet filtering method. We also introduced an improved phase-scintillation index, ? CHAIN, which we think is comparatively a better parameter to represent phase scintillations at high latitudes as the correlation between S 4 and ? CHAIN was as high as 0.90. During the analysis, we also noted that the occurrence of the "phase scintillation without amplitude scintillation" phenomenon was significantly reduced when scintillation indices were derived using the wavelet-based detrending method. These results seem to indicate that wavelet-based detrending is better suited for GPS scintillation signals and also that ? CHAIN is a better parameter for representing GPS phase scintillations at high latitudes.

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Citations
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Journal ArticleDOI

Characterization of high‐latitude ionospheric scintillation of GPS signals

TL;DR: In this article, a statistical analysis of arctic auroral oval ionospheric scintillation events during the current solar maximum based on high-rate Global Positioning System data collected in Gakona, Alaska (62.39°N, 145.15°W) from August 2010 to March 2013 is presented.
Journal ArticleDOI

Overview of the 2015 St. Patrick's day storm and its consequences for RTK and PPP positioning in Norway

TL;DR: The 2015 St. Patrick's day storm was the first storm of solar cycle 24 to reach a level of "Severe" on the NOAA geomagnetic storm scale as discussed by the authors.
Journal ArticleDOI

Comparison of the effect of high-latitude and equatorial ionospheric scintillation on GPS signals during the maximum of solar cycle 24

TL;DR: In this paper, the authors compared the characteristics of high-latitude and equatorial scintillation using multifrequency GPS data collected at Gakona, Alaska, Jicamarca, Peru, and Ascension Island during the 24th solar maximum.
Journal ArticleDOI

Climatology of GPS phase scintillation and HF radar backscatter for the high-latitude ionosphere under solar minimum conditions

TL;DR: In this article, phase scintillation is associated with auroral arc brightening and substorms or with perturbed cusp ionosphere, while the dayside scintillant patches persist over a large area of the cusp/cleft region sampled by different satellites for several hours.
References
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Journal ArticleDOI

A Practical Guide to Wavelet Analysis.

TL;DR: In this article, a step-by-step guide to wavelet analysis is given, with examples taken from time series of the El Nino-Southern Oscillation (ENSO).
Journal ArticleDOI

GPS and ionospheric scintillations

TL;DR: In this paper, the authors review the impact of scintillations on GPS receiver design and use and present a review of GPS and ionospheric scintillation for scientists interested in space weather.

Ionospheric Effects on GPS

TL;DR: In this paper, the authors describe the major effects of the ionosphere on GPS performance, including the following: 1) group delay of the signal modulation, or absolute range error, 2) carrier phase advance, or relative range error; 3) Doppler shift, or range-rate errors; 4) Faraday rotation of linearly polarized signals; 5) refraction or bending of the radio wave; 6) distortion of pulse waveforms; 7) signal amplitude fading or amplitude scintillation; and 8) phase scintillations.

Ionospheric Scintillation Monitoring Using Commercial Single Frequency C/A Code Receivers

TL;DR: The result is a design of a low-cost, portable Ionospheric Scintillation Monitor (ISM) being developed on a follow-on SBlR Phase II project and testing of a software-modified commercial C/A code receiver to perform this function.
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