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Conference paper

GPS phase scintillation and auroral electrojet currents during geomagnetic storms of March 17, 2013 and 2015

In General Assembly and Scientific Symposium of the International Union of Radio Science (ursi Gass), 2017 Xxxiind — 2017, pp. 1-4

Interplanetary coronal mass ejections (ICMEs) compounded by high-speed plasma streams from coronal holes caused two intense geomagnetic storms on March 17–18, 2013 and 2015 during the current solar cycle. Ionospheric responses to the storms in the northern and southern hemispheres are compared in the context of solar wind coupling to the magnetosphere-ionosphere system.

Phase scintillation is observed at high latitudes by arrays of high-rate GNSS Ionospheric Scintillation and TEC Monitors (GISTMs) and geodetic-quality GPS receivers sampling at 1 Hz. The high-rate GPS receivers are distributed in the northern and in the southern high latitudes with sparser coverage.

In addition to GPS receivers, the high-latitude ionosphere dynamics is studied using arrays of ground-based instruments including HF radars, ionosondes, riometers, magnetometers, optical imagers as well as particle detectors and ultraviolet scanning imagers onboard the DMSP satellites.

Language: English
Publisher: IEEE
Year: 2017
Pages: 1-4
Proceedings: XXXII General Assembly and Scientific Symposium of the International Union of Radio Science
ISBN: 1509044698 , 9082598701 , 908259871X , 9781509044696 , 9789082598704 and 9789082598711
Types: Conference paper
DOI: 10.23919/URSIGASS.2017.8105125
ORCIDs: Durgonics, Tibor

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