Zobrazeno 1 - 10
of 1 075
pro vyhledávání: '"Z. Z. Guo"'
Autor:
C. Q. Wang, H. S. Fu, J. B. Cao, Z. Wang, W. D. Fu, Z. Z. Guo, H. Lan, T. R. Sun, Y. Wei, B. B. Ni, Z. H. Yao, B. Z. Zhang
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 20, Pp n/a-n/a (2024)
Abstract Magnetic hole (MH), sometimes referred to as magnetic bottle, exhibits strong magnetic fields at its neck but weak magnetic fields at its belly. Such structure has been widely reported in the solar wind and the Earth's magnetosphere, but has
Externí odkaz:
https://doaj.org/article/083a5f7523c749f198ae9561ce0bf206
Autor:
C. Q. Wang, H. S. Fu, J. B. Cao, Z. Wang, Z. Z. Guo, W. D. Fu, Z. H. Yao, Y. Wei, B. Z. Zhang
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 8, Pp n/a-n/a (2024)
Abstract The electron rolling‐pin distribution, showing electron pitch angles primarily at 0°, 90°, and 180°, has been widely studied in the Earth's magnetosphere, but has never been reported in other planetary environments. Here, by utilizing t
Externí odkaz:
https://doaj.org/article/ddc8429cc34540ca9835d741f8fa9a99
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 2, p 155 (2024)
Magnetic holes (MHs) are transient magnetic structures responsible for energy conversion in space plasma. Using single-spacecraft measurements from Mars Atmosphere and Volatile EvolutioN (MAVEN), the existence of MHs on Mars has been confirmed. Howev
Externí odkaz:
https://doaj.org/article/951d2dcfecca48c888a2b824a7ad6340
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 2, Pp n/a-n/a (2023)
Abstract Using high‐resolution Solar Wind Electron Analyzer data from the Mars Atmosphere and Volatile EvolutioN spacecraft, we report two new types of electron pitch angle distributions (PADs) in the Martian plasma environment. The first type of e
Externí odkaz:
https://doaj.org/article/56b2614e23b841338e8ec6086138021e
Autor:
Z. Wang, X. Y. Liu, H. S. Fu, J. B. Cao, L. Dai, S. Toledo-Redondo, W. Z. Zhang, W. D. Fu, J. S. Zhao, Y. Yu, Z. Z. Guo
Publikováno v:
The Astrophysical Journal, Vol 960, Iss 1, p 45 (2023)
Reconnection fronts, also known as dipolarization fronts (DFs), and kinetic Alfvén waves (KAWs) are two of the widely observed structures and waves in the terrestrial magnetotail, but their correlation remains elusive in previous spacecraft measurem
Externí odkaz:
https://doaj.org/article/8cb65183554642b4ab45b0cf65b3e1c5
Publikováno v:
The Astrophysical Journal, Vol 960, Iss 1, p 31 (2023)
Betatron acceleration, a plasma process obtaining particle energy in the perpendicular direction but reserving energy in the field-aligned direction, is the consequence of magnetic strength enhancement when the first adiabatic invariant is conserved.
Externí odkaz:
https://doaj.org/article/5ca2c7376fa74977b70964f414cb2fc0
Publikováno v:
The Astrophysical Journal, Vol 953, Iss 1, p 34 (2023)
Magnetic discontinuities are fundamental structures in space and laboratory plasmas where the changes in magnetic and velocity fields are constrained by Rankine–Hugoniot relations. Due to the absence of precise measurements for particles, some issu
Externí odkaz:
https://doaj.org/article/c92739d2e919486fb254fd6a76aeb3ae
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 267, Iss 1, p 13 (2023)
Minimum variance analysis of the magnetic field (MVAB), among various techniques of planar structure analysis, is most widely used for its numerical simplicity and loose requirements for data. Through a large number of studies based on MVAB, a global
Externí odkaz:
https://doaj.org/article/19666bd3213c4baaad3b8ca33e06dbcf
Publikováno v:
The Astrophysical Journal, Vol 950, Iss 1, p 54 (2023)
We perform a statistical investigation of the occurrence rates of energetic electron (100–500 eV) pancake pitch-angle distributions (PADs) in the Martian space environment by utilizing 6 yr of MAVEN data. In the Martian ionosphere, we find the foll
Externí odkaz:
https://doaj.org/article/c550c94c1fc647c48836cca265870f4d
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