https://nova.newcastle.edu.au/vital/access/ /manager/Index en-au 5 https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:27694 10 keV electrons during the early recovery phase of a moderate geomagnetic storm. We find that internal energization of equatorially mirroring electrons via nonresonant ULF wave-particle interactions can explain these observations. The wave poloidal components cause radial drift of electrons, increasing (decreasing) their kinetic energy as they move inward (outward). Electrons with initial kinetic energies of a few keV can be energized to double these values within an hour by interaction with the 3 mHz waves. The energization rate is somewhat less for the 4-5 mHz waves. An increase in the ionospheric conductance decreases the power of the fast mode wave, reducing radial drift velocities and hence decreasing the rate of energization. The fast mode poloidal field varies with radial distance and longitude, and this also affects energization. Electrons which drift outward encounter a region where the toroidal field due to the field line resonance becomes dominant and produces strong azimuthal drift. These electrons become trapped in an L-shell range just outward of the resonance region and are not energized.]]> Wed 11 Apr 2018 11:43:08 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:44706 Wed 08 Mar 2023 14:35:45 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:51440 Tue 05 Sep 2023 17:57:09 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:25569 Sat 24 Mar 2018 07:35:16 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:42375 Mon 22 Aug 2022 14:29:30 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:39700 Fri 17 Jun 2022 16:35:05 AEST ]]>