Spectacular auroras were spotted at unusual latitudes in China during a severe geomagnetic storm.
CN-DARN reveals the link of auroral intensification to dawnside subauroral polarization (SAPS) streams.
CN-DARN observed high-speed ionospheric irregularities driven by dawnside SAPS invading China’s airspace.
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The fields-of-view (FOVs) of the six CN-DARN radars and the variation of the geomagnetic coordinates for the Siziwang Observatory of Space Weather (SOSW)
Solar wind conditions and geomagnetic indices during 10-11 October 2024
The auroral images captured from the Siziwang Observatory of Space Weather in Inner Mongolia, China
Ionospheric total electron content (TEC) retrieved from global GNSS receivers at (A)
Range-time-intensity (RTI) plots of the ionospheric irregularities LOS velocity observed from CN-DARN radars
One-minute plots of the LOS velocity of ionospheric irregularities observed by four CN-DARN radars versus magnetic latitude and magnetic local time for (A) 1858 UT, (B) 1944 UT, (C) 2036 UT, and (D)
Two snapshots of the Northern Hemisphere ionospheric convection maps on October 10, 2024
Auroral radio absorption detected by Siziwang West radar on October 10, 2024