Zobrazeno 1 - 10
of 411
pro vyhledávání: '"Zhonghua Yao"'
Publikováno v:
地球与行星物理论评, Vol 55, Iss 6, Pp 638-651 (2024)
The internal structure and dynamics of different planets are different, so some planets have an intrinsic magnetic field, and some have not yet found an intrinsic magnetic field. A planet's intrinsic magnetic field or atmosphere interacts with the so
Externí odkaz:
https://doaj.org/article/9a98f0536d5b4c309cdb9c58992ab9d6
Publikováno v:
Earth and Planetary Physics, Vol 8, Iss 5, Pp 703-710 (2024)
Jupiter is one of the top priorities for deep space exploration in China and other countries. The structure of Jupiter’s interior, in particular, is a crucial but still unclear scientific topic. This paper discusses current scientific understanding
Externí odkaz:
https://doaj.org/article/99882e9471d14dbb9a19d5cda65eeb9c
Autor:
ZhongHua Yao, RuiLong Guo, Yong Wei, Bertrand Bonfond, Denis Grodent, BinZheng Zhang, William R. Dunn, ZuYin Pu
Publikováno v:
Earth and Planetary Physics, Vol 8, Iss 5, Pp 659-672 (2024)
Magnetic reconnection and dipolarization are crucial processes driving magnetospheric dynamics, including particle energization, mass circulation, and auroral processes, among others. Recent studies have revealed that these processes at Saturn and Ju
Externí odkaz:
https://doaj.org/article/956f879926d24940965752f75d5b93d4
Statistical Analysis of Whistler Precursors Upstream of Foreshock Transient Shocks: MMS Observations
Autor:
Mengmeng Wang, Terry Z. Liu, Hui Zhang, Kaijun Liu, Quanqi Shi, Ruilong Guo, Anmin Tian, Weijie Sun, Xiao‐Chen Shen, Siyuan Wu, Alexander W. Degeling, Yan Wang, Shi‐Chen Bai, Zhonghua Yao, Wenya Li, Shuai Zhang, Timo Pitkänen, Shutao Yao, Ji Liu, Kun Cheng, Xiao Ma, Yuqi Liu
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 8, Pp n/a-n/a (2024)
Abstract Using the high‐time‐resolution data from the Magnetospheric Multiscale mission, precursor waves upstream of foreshock transient (FT) shocks are statistically investigated using the four‐spacecraft timing method. The wave frequencies an
Externí odkaz:
https://doaj.org/article/27e0ffa5cee74472b7e76283fb8c8389
Publikováno v:
地球与行星物理论评, Vol 54, Iss 5, Pp 541-557 (2023)
The coupling between solar wind and the magnetosphere and the dynamic processes in geo-space are the basic driving factors of space weather. Understanding these processes on the system level is essential to the studies of space physics and space weat
Externí odkaz:
https://doaj.org/article/8da1db1487b24d3889496ed41d1733de
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
In this study, we explore the evolution of long-duration transpolar arcs observed during an exceptionally quiet period by the Fengyun-3D and Defense Meteorological Satellite Program satellites on 17 January 2019. Leveraging the extensive field of vie
Externí odkaz:
https://doaj.org/article/3237b1474197406e8236b8d84fe86f05
Publikováno v:
Earth and Planetary Physics, Vol 7, Iss 3, Pp 414-420 (2023)
A mirror mode wave is a fundamental magnetic structure in the planetary space environment that is persistently compressed by solar wind, especially in the magnetosheath. Mirror modes have been widely identified in the magnetosheaths of the Earth and
Externí odkaz:
https://doaj.org/article/8c67855bf9314a7d9866efa63b7c04da
Autor:
Fei He, ZhongHua Yao, BinBin Ni, Xing Cao, ShengYi Ye, RuiLong Guo, JinXing Li, ZhiPeng Ren, XinAn Yue, YongLiang Zhang, Yong Wei, XiaoXin Zhang, ZuYin Pu
Publikováno v:
Earth and Planetary Physics, Vol 7, Iss 2, Pp 237-246 (2023)
The dune aurora, at a scale of ~30 kilometers, was reported recently using ground camera. The small-scale dune aurora occurs on the duskside and exhibits a monochromatic oscillation in the auroral emission, implying fundamental energy conversions. Ho
Externí odkaz:
https://doaj.org/article/9bbd50b3c01c4f14889f116ddc5a2d5e
Publikováno v:
Earth and Space Science, Vol 10, Iss 11, Pp n/a-n/a (2023)
Abstract Characterizing the temporal evolution of the three‐dimensional structure of the Io plasma torus is essential to understand the dynamics of the Jovian magnetosphere. Optical imaging is a powerful tool to uncover the global torus structure.
Externí odkaz:
https://doaj.org/article/05b04c3a78e945b5bdd97547344b4d0c
Autor:
Minyi Long, Xing Cao, Binbin Ni, Yuequn Lou, Zhonghua Yao, Elias Roussos, Tianshu Qin, Siyuan Wu
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 19, Pp n/a-n/a (2023)
Abstract The features of electron pitch angle distributions (PADs) often imply different physical mechanisms in planetary magnetospheres. We report a simultaneous equatorial electrostatic electron cyclotron harmonic (ECH) wave event with butterfly PA
Externí odkaz:
https://doaj.org/article/088ab68d3e0e49d797ea3acfe8d0ce36