GPS TEC variations in the polar cap ionosphere: Solar wind and IMF dependence. Issue 9 (17th September 2016)

• Record Type: Journal Article
• Authors: Watson, Chris; Jayachandran, P. T.; MacDougall, John W.
• Is Part Of: Journal of geophysical research. Volume 121:Issue 9(2016:Sep.)
• Page Start: 9030
• Page End: 9050
• Publication Date: 2016-09-17
• Subjects: GPS -- TEC -- polar cap -- ionosphere -- solar wind -- IMF; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1002/2016JA022937
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: This statistical study examines the solar wind dependence of total electron content (TEC) variations arising from mesoscale (tens to hundreds of kilometers) structuring of the polar cap ionosphere. Six years of TEC measurements were collected from five high‐data rate Global Positioning System (GPS) receivers of the Canadian High Arctic Ionospheric Network (CHAIN), from which high‐resolution magnetic local time‐latitude maps of TEC variation occurrence rate and amplitude were created. Ionosonde radars were used to identify TEC variations arising from ionization of the E and F region ionospheres. Statistical TEC maps were examined as a function of solar wind and interplanetary magnetic field (IMF) measurements. Statistical results showed that occurrence rate of TEC variations was highest in localized dayside regions, with exact local time and latitude of peak occurrence depending primarily on the dayside coupling rate of the solar wind and magnetosphere, as well as IMF orientation and magnitude in the Y‐Z plane. Occurrence of TEC variations throughout the polar cap increased with solar wind‐magnetosphere coupling rate and IMF magnitude. The solar wind dependence of occurrence rate largely reflected the location and rate of dayside magnetic reconnection and subsequent particle precipitation and polar cap convection. Amplitudes of TEC variations were largest around noon and increased throughout the polar cap with increased solar wind‐magnetosphere coupling rate. These statistical results improve upon the existing observational picture of the polar ionosphere and will potentially facilitate development of models and techniques for mitigating impacts of the polar ionosphere on navigation signals and communication links. Key Points: Occurrence rate of polar cap TEC variations increased with dayside solar wind‐magnetosphere coupling rate and IMF magnitude Local time and latitude of peak occurrence rates varied with IMF BY and BZ Average amplitude of polar cap TEC variations increased with solar wind‐magnetosphere coupling rate