Prikryl, PaulGillies, Robert G.Themens, David R.Weygand, James M.Thomas, Evan G.Chakraborty, Shibaji2023-04-242023-04-242022-11http://hdl.handle.net/10919/114765During minor to moderate geomagnetic storms, caused by corotating interaction regions (CIRs) at the leading edge of high-speed streams (HSSs), solar wind Alfven waves modulated the magnetic reconnection at the dayside magnetopause. The Resolute Bay Incoherent Scatter Radars (RISR-C and RISR-N), measuring plasma parameters in the cusp and polar cap, observed ionospheric signatures of flux transfer events (FTEs) that resulted in the formation of polar cap patches. The patches were observed as they moved over the RISR, and the Canadian High-Arctic Ionospheric Network (CHAIN) ionosondes and GPS receivers. The coupling process modulated the ionospheric convection and the intensity of ionospheric currents, including the auroral electrojets. The horizontal equivalent ionospheric currents (EICs) are estimated from ground-based magnetometer data using an inversion technique. Pulses of ionospheric currents that are a source of Joule heating in the lower thermosphere launched atmospheric gravity waves, causing traveling ionospheric disturbances (TIDs) that propagated equatorward. The TIDs were observed in the SuperDual Auroral Radar Network (SuperDARN) high-frequency (HF) radar ground scatter and the detrended total electron content (TEC) measured by globally distributed Global Navigation Satellite System (GNSS) receivers.application/pdfenCreative Commons Attribution 4.0 InternationalInterplanetary magnetic-fieldatmospheric gravity-wavesflux-transfer eventsdissipative multiconstituent mediumhigh-latitude ionosphereradar observationsinteraction regionsglobal propagationf-regionrisr-cArticle - Refereedhttps://doi.org/10.5194/angeo-40-619-20224061432-0576