Zobrazeno 1 - 10
of 1 452
pro vyhledávání: '"H. S. Fu"'
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
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 20, Pp n/a-n/a (2024)
Abstract The tailward high‐speed flows, in which various kinetic processes and magnetic structures can be embedded, are usually produced by the magnetic reconnection in the Earth's magnetotail. Here, using high‐resolution measurements from the Ma
Externí odkaz:
https://doaj.org/article/6426e6dbbbdd438aa2fd01e7d4252fc2
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 16, Pp n/a-n/a (2024)
Abstract Anti‐dipolarization fronts (ADFs), characterized by the rapid increase of the negative magnetic field Bz component, are typically formed at the leading edge of the tailward reconnection jets in the Earth's magnetotail. To date, the electro
Externí odkaz:
https://doaj.org/article/20021b9bd9e544159fda1cb585b1b258
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:
Physical Review Research, Vol 6, Iss 1, p L012047 (2024)
A whistler wave is a fundamental electromagnetic radiation. In the universe, it transmits information through diverse mediums at audio frequencies. To know the properties of such a radio, one should determine how its frequency (energy) changes with i
Externí odkaz:
https://doaj.org/article/a1bf3119b3ab4c50ab2a27ec1bdf2f58
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 24, Pp n/a-n/a (2023)
Abstract The Earth's magnetopause is an ion‐scale boundary that separates the magnetosphere from the shocked solar wind. At such boundary, energy‐conversion processes frequently occur. Previous studies suggested that such energy conversions are r
Externí odkaz:
https://doaj.org/article/85311704e4bc4b58ba6cba4b6a81ad8e
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 17, Pp n/a-n/a (2023)
Abstract The electron butterfly distribution, characterized by pitch angles (PA) primarily at 45° and 135°, was rarely observed in Earth's magnetotail. Here using the high‐resolution measurements from Magnetospheric Multiscale mission, we present
Externí odkaz:
https://doaj.org/article/3db530dbad5141b0ab7343a0977ac5e2
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:
The Astrophysical Journal, Vol 963, Iss 1, p 64 (2024)
Space plasmas are turbulent and maintain different types of critical points or flow nulls. Electron vortex, as one type of flow null structure, is crucial in the energy cascade in turbulent plasmas. However, due to the limited time resolution of the
Externí odkaz:
https://doaj.org/article/25ee4c7c4c274afd9bd16cbb201dd02c
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