Differentiating between the leading processes for electron radiation belt acceleration
Many spacecraft fly within or through a natural and variable particle accelerator powered by
the coupling between the magnetosphere and the solar wind: the Earth's radiation belts …
the coupling between the magnetosphere and the solar wind: the Earth's radiation belts …
The radiation belts of Jupiter and Saturn
E Roussos, P Kollmann - Magnetospheres in the solar system, 2021 - Wiley Online Library
The era of outer planet orbiters (Galileo, Juno and Cassini) is advancing our understanding
of how the radiation belts of Jupiter and Saturn are structured, form, and evolve well beyond …
of how the radiation belts of Jupiter and Saturn are structured, form, and evolve well beyond …
Saturn's inner magnetospheric convection in the view of zebra stripe patterns in energetic electron spectra
Banded structures observed in energetic particle spectrograms in the Earth's inner radiation
belt and slot region, that is,“zebra stripes,” have been resolved in the Saturnian …
belt and slot region, that is,“zebra stripes,” have been resolved in the Saturnian …
Highlight Advances in Planetary Physics in the Solar System: In Situ Detection Over the Past 20 Years
Planetary science is the science of studying planets, moons, and planetary systems. The
scale of the research objects ranges from small meteoroids to large gas giant planets, and …
scale of the research objects ranges from small meteoroids to large gas giant planets, and …
Zebra stripe patterns in energetic ion spectra at Saturn
Magnetospheric convective electric fields that could radially transport particles adiabatically,
may leave their imprints in the form of energy‐time dispersed patterns termed” zebra …
may leave their imprints in the form of energy‐time dispersed patterns termed” zebra …
Cassini observation of relativistic electron butterfly distributions in Saturn's inner radiation belts: Evidence for acceleration by local processes
The morphology of electron pitch angle distributions (PADs) helps to identify dynamic
processes in Saturn's magnetosphere. Previous studies demonstrated convective transport …
processes in Saturn's magnetosphere. Previous studies demonstrated convective transport …
Quantifying the absorption loss of radiation belt energetic particles by Saturn's inner moons
Saturn owns various moons embedded in the magnetosphere, which results in the
absorption loss of energetic particles in Saturn's radiation belts when they encounter the …
absorption loss of energetic particles in Saturn's radiation belts when they encounter the …
[HTML][HTML] Magnetospheric Physics in China: 2020–2021
CAO Jinbin, Y Junying - 空间科学学报, 2022 - cjss.ac.cn
In the past two years, many progresses were made in magnetospheric physics by the data of
OMNI, SuperMAG networks, Double Star Program, Cluster, THEMIS, RBSP, DMSP …
OMNI, SuperMAG networks, Double Star Program, Cluster, THEMIS, RBSP, DMSP …
Large‐scale episodic enhancements of relativistic electron intensities in Jupiter's radiation belt
Previous studies indicate that, in the Jovian magnetosphere, the long‐term trend of the
radial profile of relativistic electron intensities is primarily shaped by slow radial diffusion …
radial profile of relativistic electron intensities is primarily shaped by slow radial diffusion …
巨行星空间环境研究进展
尧中华， 郭瑞龙， 袁憧憬， 潘东晓， 许严 - 地球与行星物理论评, 2021 - sjdz.org.cn
太阳系八大行星分为类地行星和巨行星, 巨行星不仅体积和质量大, 其磁场也相对更强.
土星的磁矩大约是地球的600 倍, 而木星的磁矩则有地球的20 000 倍之大 …
土星的磁矩大约是地球的600 倍, 而木星的磁矩则有地球的20 000 倍之大 …