Explaining the dynamics of the sub-relativistic electron third belt in the Earth's radiation belts by using medium Earth orbit satellite observationsOAEI
Explaining the dynamics of the sub-relativistic electron third belt in the Earth's radiation belts by using medium Earth orbit satellite observations
The Earth's electron radiation belts typically exhibit a two-belt structure.However,observations from the Van Allen Probes revealed the existence of a three-belt structure.This structure consists of an inner belt,a slot region,a remnant belt,a"second slot,"and a new outer belt(or the"third belt").The formation of the structure involves both the partial loss of the original outer belts and the formation of the third belts.These processes are likely associated with radial diffusion induced by ultra-low-frequency(ULF)waves.In this study,we mainly analyzed electron flux data from medium Earth orbit(MEO)navigation satellites M17-M19 to supplement the observational evidence for the sub-relativistic electron(～100-500 keV)three-belt structure.Evidence of substorm injections and ULF waves during the three-belt event was identified,suggesting they played significant roles in the formation and evolution of the third belt.Substorm injections may introduce new electron populations to the third belt,whereas ULF waves may influence the evolution of the third belt through radial diffusion.Toward the end of the three-belt event,the compression of the magnetosphere by shocks may lead to the dropout of the third belt because of the magnetopause shadowing effect and outward radial diffusion,ultimately disrupting the three-belt structure.This study provides more evidence for the presence of a sub-relativistic electron three-belt structure and offers an analysis of the evolutionary mechanisms of the third belt,which may contribute to a comprehensive understanding of the electron three-belt structure in the radiation belts.
JiaLi Chen;Hong Zou;YuGuang Ye
Institute of Space Physics and Applied Technology,Peking University,Beijing 100871,China
third beltsub-relativistic electronsthree-belt structureradiation beltsmagnetic storms and substormswave-particle interactions
《地球与行星物理（英文）》 2024 (005)
762-775 / 14
The M17-M19 MES and HED data can be obtained by contacting the corresponding author.The NOAA-18 MEPED data were provided by NASA's Space Physics Data Facility(https://cdaweb.gsfc.nasa.gov/pub/data/noaa/noaa18/sem2_fluxes-2sec/2020/).The IMF,solar wind dynamic pressure,solar wind velocity,and SYM-H data were obtained from the NASA OMNI database(https://omniweb.gsfc.nasa.gov/).The SME data were provided by SuperMAG collaboration(https://supermag.jhuapl.edu/mag/?fidelity=low&start=2001-01-29T16％3A00％3A00.000Z&interval=23％3A59).The ERG MGF and orbit data can be down-loaded from the ERG Science Center(https://ergsc.isee.nagoya-u.ac.jp/).The authors thank the NOAA-18 team,NASA's Space Physics Data Facility,the SuperMAG collaboration,and the ERG team for providing valuable data.This work was supported by the National Natural Science Foundation of China(Grant No.42274225).
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