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Journal ArticleDOI

GPS scintillation in the high arctic associated with an auroral arc

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TLDR
In this article, the authors show that at high latitudes low-elevation GPS signals can suffer sudden fading due to E-region auroral events and that the signal fades can be attributed to the GPS ray paths crossing electron density structures associated with the aurora.
Abstract
A rapid signal-fading event produced by diffractive scintillations was observed around 0123 UT on 8 November 2004 by three closely sited (less than 250 m apart) GPS scintillation receivers in northern Norway. The entire duration of the event was about 10 s and was recorded by all three receivers. Intense, short duration events such as these are not clearly observable in the 1-min scintillation index (S4) because they do not necessarily last for the entire minute. In spite of their short duration they can cause a receiver to lose lock because of their intensity. The geomagnetic conditions were disturbed at this time with the interplanetary magnetic field southward for a period of several hours. Magnetometers from the IMAGE network in Scandinavia showed evidence of a 2000 nT substorm. The GPS measurements are compared with all-sky camera (ASC) data to show that the signal fades can be attributed to the GPS ray paths crossing electron density structures associated with the aurora. The ASC images reveal moving auroral structures at the same time as the GPS signals show movement of the ionospheric regions causing fading. The results indicate that at high latitudes low-elevation GPS signals can suffer sudden fading due to E-region auroral events. This is the first time that a direct connection has been established between the loss of lock on a GPS receiver and diffractive fading caused by auroral precipitation.

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The MAVEN EUVM model of solar spectral irradiance variability at Mars: Algorithms and results

TL;DR: In this article, an iteration of the FISM model called Flare Irradiance Spectral Model (FISM-M) was used to estimate the solar extreme ultraviolet (EUV) radiation at Mars.
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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.
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Solar flares, coronal mass ejections and solar energetic particle event characteristics

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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.
References
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Book

Communication Systems

Simon Haykin
TL;DR: This best-selling, easy to read book offers the most complete discussion on the theories and principles behind today's most advanced communications systems.

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.
Journal ArticleDOI

Ionospheric constraints on VHF/UHF communications links during solar maximum and minimum periods

TL;DR: In this article, an extensive VHF/UHF scintillation data base covering the frequency range of VHF to a few gigahertz has been utilized to determine the magnitudes of phase and intensity scintillations and their temporal/spatial structures during the sunspot maximum and minimum periods.
Journal ArticleDOI

Specification and forecasting of scintillations in communication/navigation links: current status and future plans

TL;DR: In this paper, a global specification and forecast system for scintillation is needed in view of our increased reliance on space-based communication and navigation systems, which are vulnerable to ionospheric scintillations.
Journal ArticleDOI

Ionospheric effects of major magnetic storms during the International Space Weather Period of September and October 1999: GPS observations, VHF/UHF scintillations, and in situ density structures at middle and equatorial latitudes

TL;DR: In this article, the ionospheric effects of a halo coronal mass ejection (CME) initiated on the Sun on September 20, 1999, and causing the largest magnetic storm during this month on September 22, 23, and 24, 1999 were studied through their effects on a prototype of a Global Positioning System (GPS)-based navigation system called Wide Area Augmentation System (WAAS) and their impact on global VHF/UHF communication systems.
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