https://ogma.newcastle.edu.au/vital/access/ /manager/Index en-au 5 https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:16990 Wed 11 Apr 2018 13:08:58 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:16991 Wed 11 Apr 2018 09:45:23 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:33035 y, indicating a connection between the R1 fluctuation and the driving solar wind most likely explained by magnetic reconnection; and (4) high‐frequency fluctuations in R2 are enhanced in a small region near local noon and respond clearly to nightside drivers, as characterized by the auroral electrojet index. Our analysis shows that the intensity of R1 and R2 high‐frequency magnetic fluctuations is directly connected to the intensity of FACs, which implies that the magnetic fluctuations are closely related to the magnetospheric processes that drive them.]]> Tue 03 Sep 2019 18:23:38 AEST ]]>