Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/42656
Title: Experimental Evidence on the Dependence of the Standard GPS Phase Scintillation Index on the Ionospheric Plasma Drift Around Noon Sector of the Polar Ionosphere
Authors: Wang, Y.
Zhang, Q.-H.
Jayachandran, P. T.
Moen, J.
Xing, Z.-Y.
Chadwick, R.
Ma, Y.-Z.
Ruohoniemi, J. M.
Lester, M.
First Published: 8-Mar-2018
Publisher: American Geophysical Union (AGU), Wiley
Citation: Journal of Geophysical Research: Space Physics, 2018, 123 (3), pp. 2370-2378 (9)
Abstract: First experimental proof of a clear and strong dependence of the standard phase scintillation index (σφ) derived using Global Positioning System measurements on the ionospheric plasma flow around the noon sector of polar ionosphere is presented. σφ shows a strong linear dependence on the plasma drift speed measured by the Super Dual Auroral Radar Network radars, whereas the amplitude scintillation index (S4) does not. This observed dependence can be explained as a consequence of Fresnel frequency dependence of the relative drift and the used constant cutoff frequency (0.1 Hz) to detrend the data for obtaining standard σφ. The lack of dependence of S4 on the drift speed possibly eliminates the plasma instability mechanism(s) involved as a cause of the dependence. These observations further confirm that the standard phase scintillation index is much more sensitive to plasma flow; therefore, utmost care must be taken when identifying phase scintillation (diffractive phase variations) from refractive (deterministic) phase variations, especially in the polar region where the ionospheric plasma drift is much larger than in equatorial and midlatitude regions.
DOI Link: 10.1002/2017JA024805
ISSN: 2169-9380
eISSN: 2169-9402
Links: https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1002/2017JA024805
http://hdl.handle.net/2381/42656
Embargo on file until: 8-Sep-2018
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2018, American Geophysical Union (AGU), Wiley. Deposited with reference to the publisher’s open access archiving policy. (http://www.rioxx.net/licenses/all-rights-reserved)
Description: The file associated with this record is under embargo until 6 months after publication, in accordance with the publisher's self-archiving policy. The full text may be available through the publisher links provided above.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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