Conference paper
GPS phase scintillation during the geomagnetic storm of March 17, 2015: The relation to auroral electrojet currents
University of New Brunswick1
Natural Resources Canada2
Athabasca University3
University of California at Los Angeles4
Virginia Polytechnic Institute and State University5
National Space Institute, Technical University of Denmark6
Geodesy, National Space Institute, Technical University of Denmark7
University of Bergen8
Johns Hopkins University9
Ionospheric irregularities cause rapid fluctuations of radio wave amplitude and phase that candegrade GPS positional accuracy and affect performance of radio communication and navigation systems. The ionosphere becomes particularly disturbed during geomagnetic storms caused by impacts of coronal mass ejections compounded by high-speed plasma streams from coronal holes.
Geomagnetic storm of March 17, 2015 was the largest in the current solar cycle. The high-latitude ionosphere dynamics is studied using arrays of ground-based instruments including GPS receivers, HF radars, ionosondes, riometers and magnetometers. GPS phase scintillation index is computed for L1 signal sampled at the rate of 50 Hz by specialized GPS scintillation receivers of the Expanded Canadian High Arctic Ionospheric Network (ECHAIN).
To further extend the geographic coverage, the phasescintillation proxy index is obtained from geodetic-quality GPS data sampled at 1 Hz. In the context of solar wind coupling to the magnetosphere-ionosphere system, it has been demonstrated that GPS phase scintillation is primarily enhanced in the cusp, tongue of ionization (TOI) broken into patches drawn into the polar cap from the dayside storm-enhanced plasma density (SED) and in the auroral oval during energetic particle precipitation events, substorms and pseudo-breakups in particular.
In this paper we examine the relation to auroral electrojet currents observed by arrays of ground-based magnetometers and energetic particle precipitation observed by DMSP satellites. Equivalent ionospheric currents (EICs) are obtained from ground magnetometer data using the spherical elementary currents systems (SECS) technique developed by Amm and Viljanen (1999) that has been applied over the entire North American ground magnetometer network by Weygand et al.(2011).
Language: | English |
---|---|
Year: | 2016 |
Proceedings: | Japan Geoscience Union Meeting 2016 |
Types: | Conference paper |
ORCIDs: | Durgonics, Tibor |