GPS and ionospheric scintillations

By Paul M. Kintner, B. Ledvina, E. R. D. Paula. 2007

655 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/1b7c170eb5c5f461c143d6328d89490f30aff290

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Citations in the corpus

• Improved amplitude- and phase-scintillation indices derived from wavelet detrended high-latitude GPS data (2012, background): “Scintillation has an important place in ionospheric research since it gives information about the smallscale electron density structures present in the ionosphere (Basu et al. 1988; Kintner et al. 2007; MacDougall and Jayachandran 2007; Strangeways 2009).”
• Comparison of the effect of high‐latitude and equatorial ionospheric scintillation on GPS signals during the maximum of solar cycle 24 (2015, background): “Research also shows that equatorial scintillation is more frequent and intense around equinoxes and subsides in the summer [Aarons, 1982; Tsunoda, 1985; Kintner et al., 2007; Beniguel et al., 2009].”
• Canadian High Arctic Ionospheric Network (CHAIN) (2009, methodology): “(For more on GPS and scintillations, see Kintner et al. [2007] .) However, recent scintillation studies based on GPS data were conducted for extreme magnetic storm conditions [Mitchell et al., 2005; Meggs et al., 2008].”
• Characterization of high‐latitude ionospheric scintillation of GPS signals (2013, background): “Occurrence of scintillation is difficult to predict and model because of the temporal and spatial variability of the ionosphere and solar activities that are driving forces of space weather phenomena [Kintner et al., 2007].”
• Space weather challenges of the polar cap ionosphere (2017, background): “1988a, 1998), but may occur at any place or time during the entire solar cycle (Kintner et al. 2007).”