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- W2022285495 abstract "Convection data from SuperDARN radars in the northern hemisphere are utilized to investigate the response of high-latitude ionospheric convection during a southward IMF turning event, focused on the response timescale. In this event, IMF Bz component changed from +7 nT to –8 nT in 1.5 min and had been relatively stable for 40 min before and after the IMF turning, respectively. The initial ionospheric convection response started near magnetic local noon about 3 min after the IMF turning. The response was delayed by increasing amounts away from noon. The delay of the convection response is about 6 min around dawn and dusk, and 12 min around midnight. There is no clear MLT dependence for the reconfiguration time of the convection response and such timescale is 10~14 min." @default.
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- W2022285495 date "2007-11-01" @default.
- W2022285495 modified "2023-09-26" @default.
- W2022285495 title "The Response of High-Latitude Ionospheric Convection During a Southward IMF Turning Event" @default.
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- W2022285495 doi "https://doi.org/10.1002/cjg2.1159" @default.
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