Zobrazeno 1 - 10
of 171
pro vyhledávání: '"S.-D. Xiao"'
Publikováno v:
Earth, Planets and Space, Vol 73, Iss 1, Pp 1-9 (2021)
Abstract We statistically investigate the spectral scalings of magnetic fluctuations at the upstream and downstream regions near the Venusian bow shock and perform a differentiation by shock geometry. Based on the Venus Express data, 115 quasi-parall
Externí odkaz:
https://doaj.org/article/06d8cf57389d4afa985f753dd135be21
Autor:
Z. Zhang, E. H. Wang, S. J. Zhu, J. H. Hamilton, A. V. Ramayya, J. K. Hwang, R. Q. Xu, Z. Jiang, S. D. Xiao, X. Q. Zhang, J. Kormicki, P. M. Gore, E. F. Jones, W. C. Ma, J. D. Cole, M. W. Drigert, I. Y. Lee, J. O. Rasmussen, Y. X. Luo, T. N. Ginter, C. Folden, P. Fallon, P. Zielinski, K. E. Gregorich, A. O. Macchiavelli, R. Donangelo, M. A. Stoyer
Publikováno v:
Physical Review C. 106
Publikováno v:
Journal of Geophysical Research: Space Physics. 127
Publikováno v:
Journal of Geophysical Research: Space Physics. 127
Autor:
G. Q. Wang, Martin Volwerk, S. D. Xiao, Geli Wang, T. L. Zhang, Yukuan Chen, Jicheng Sun, Mingyu Wu
Publikováno v:
Geophysical Research Letters. 48
Publikováno v:
The Astrophysical Journal. 927:171
One Martian induced magnetosphere boundary (IMB) crossing at the subsolar region is analyzed here with multiple instruments on board MAVEN. Properties of the magnetic field and particles around the IMB are evaluated. We find different trends of varia
Publikováno v:
The Astrophysical Journal. 921:153
Publikováno v:
The Astrophysical Journal. 921:152
Publikováno v:
Journal of Geophysical Research: Space Physics. 122:8858-8867
We investigate the characteristics of the magnetic flux rope in the Venusian ionosphere near the terminator observed by the Venus Express while previous works about flux rope by PVO are mainly in the subsolar region. The probability to observe the fl
Publikováno v:
Journal of Geophysical Research: Space Physics. 122:8409-8418
We statistically investigate the solar cycle dependence of the magnetic field fluctuations in the frequency range 30-300 mHz based on Venus Express data. We present the spatial distributions of fluctuation properties during three typical periods of t