Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Chongjing Yuan"'
Autor:
Chi Zhang, Hans Nilsson, Yusuke Ebihara, Masatoshi Yamauchi, Moa Persson, Zhaojin Rong, Jun Zhong, Chuanfei Dong, Yuxi Chen, Xuzhi Zhou, Yixin Sun, Yuki Harada, Jasper Halekas, Shaosui Xu, Yoshifumi Futaana, Zhen Shi, Chongjing Yuan, Xiaotong Yun, Song Fu, Jiawei Gao, Mats Holmström, Yong Wei, Stas Barabash
Publikováno v:
Nature Communications, Vol 14, Iss 1, Pp 1-10 (2023)
Abstract Mars lacks a global magnetic field, and instead possesses small-scale crustal magnetic fields, making its magnetic environment fundamentally different from intrinsic magnetospheres like those of Earth or Saturn. Here we report the discovery
Externí odkaz:
https://doaj.org/article/5a4393e0c82b4a9b9b22b96159007e59
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 1, Pp n/a-n/a (2024)
Abstract In Jupiter's middle magnetosphere, debate remains on the controlling physics of electron acceleration to the ultrarelativistic regime. Some local‐time asymmetric processes regulating MeV electrons may have their hold across electron spectr
Externí odkaz:
https://doaj.org/article/1361e918e96b4166984d19e64ae3859e
Publikováno v:
地球与行星物理论评, Vol 52, Iss 5, Pp 543-560 (2021)
Among the eight solar system planets, Jupiter and Saturn are the two most giant planets, which also have the most prominent magnetic moments. Comparing to the Earth dipole magnetic field, the magnetic moment of Saturn is about 600 times larger while
Externí odkaz:
https://doaj.org/article/d340c02cae2c4a41a3c969e99ff2b334
Publikováno v:
Earth and Planetary Physics, Vol 5, Iss 4, Pp 314-326 (2021)
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. However, measurements by the Galileo spacecraft reveal the exist
Externí odkaz:
https://doaj.org/article/055972b7422d411bab9eb73ebe2208b0
The solar wind plasma upstream of Mars observed by Tianwen-1: Comparison with Mars Express and MAVEN
Autor:
Kai Fan, Limei Yan, Yong Wei, Aibing Zhang, Linggao Kong, Markus Fränz, Fei He, Lihui Chai, Chongjing Yuan, Yuqi Wang, Jun Zhong, Zhaojin Rong, Zhonghua Yao, Yongxin Pan, Jun Cui, Jiansen He, Wenya Li, Binbin Tang, Chi Wang
Publikováno v:
Science China Earth Sciences. 65:759-768
Autor:
Zhen Shi, Zhaojin Rong, Shahab Fatemi, James A. Slavin, Lucy Klinger, Chuanfei Dong, Liang Wang, Jun Zhong, Jim M Raines, Mats Holmström, Chongjing Yuan, Stas Barabash, Yong Wei
Publikováno v:
Geophysical Research Letters. 49
Mercury has a terrestrial-like magnetosphere which is usually taken as a scaled-down-version of Earth's magnetosphere with a similar current system. We examine Mercury's magnetospheric current system based on a survey of Mercury's magnetic field meas
Publikováno v:
Earth and Planetary Physics. 5:1-13
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. However, measurements by the Galileo spacecraft reveal the exist
Publikováno v:
Geophysical Research Letters. 48
Autor:
Chongjing Yuan, Q.-G. Zong
Publikováno v:
Journal of Geophysical Research: Space Physics. 124:3222-3235
Autor:
Peter Kollmann, Yixin Hao, Ying Liu, Norbert Krupp, H. Kita, Chris Paranicas, Elias Roussos, Chongjing Yuan, Xu-Zhi Zhou, Qiugang Zong, Go Murakami, Yixin Sun
The existence of planetary radiation belts with relativistic electron components means that powerful acceleration mechanisms are operating within their volume. Mechanisms that bring charged particles planetward toward stronger magnetic fields can cau
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9bda0af103ec79ecf8289e0a067e40a9
https://doi.org/10.5194/egusphere-egu21-8779
https://doi.org/10.5194/egusphere-egu21-8779