Explaining the dynamics of the sub-relativistic electron third belt in the Earth's radiation belts by using medium Earth orbit satellite observations
Explaining the dynamics of the sub-relativistic electron third belt in the Earth's radiation belts by using medium Earth orbit satellite observations
摘要
关键词
third belt/sub-relativistic electrons/three-belt structure/radiation belts/magnetic storms and substorms/wave-particle interactionsKey words
third belt/sub-relativistic electrons/three-belt structure/radiation belts/magnetic storms and substorms/wave-particle interactions引用本文复制引用
JiaLi Chen,Hong Zou,YuGuang Ye..Explaining the dynamics of the sub-relativistic electron third belt in the Earth's radiation belts by using medium Earth orbit satellite observations[J].地球与行星物理（英文）,2024,8(5):762-775,14.基金项目
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). （https://cdaweb.gsfc.nasa.gov/pub/data/noaa/noaa18/sem2_fluxes-2sec/2020/）
