Results 11 to 20 of about 3,124 (266)
Bow shock oscillations of Mars under weakly disturbed solar wind conditions [PDF]
Nature CommunicationsBow shock, where the solar wind first encounters the Martian environment, reflects the complex interplay between the solar wind and Martian upper atmosphere and crustal fields.
Long Cheng +15 more
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Properties and models of the Martian bow shock
地球与行星物理论评, 2021 Mars does not have a global magnetic field of the internal origin, thus, the solar wind plasma can interact directly with the upper atmosphere and the ionosphere and be shocked with the mass-loading and magnetic pileup processes.
Yifan Li +4 more
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The spectral scalings of magnetic fluctuations upstream and downstream of the Venusian bow shock
Earth, Planets and Space, 2021 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.
S. D. Xiao +4 more
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THE RETURN OF THE BOW SHOCK [PDF]
The Astrophysical Journal, 2014 Recently it has been discussed whether a bow shock ahead of the heliospheric stagnation region does exist or not. This discussion was triggered by measurements indicating that the Alfvén speed and that of fast magnetosonic waves are higher than the flow speed of the local interstellar medium (LISM) relative to the heliosphere and resulted in the ...
Scherer, Klaus, Fichtner, Horst
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Frontiers in Astronomy and Space Sciences, 2023 On the bow shock in front of Earth’s magnetosphere flows a current due to the curl of the interplanetary magnetic field across the shock. The closure of this current remains uncertain; it is unknown whether the bow shock current closes with the Chapman ...
Pauline M. Dredger +2 more
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Geophysical Research Letters, 2021 Collisionless shocks can be nonstationary with periodic reformation shown in many simulation results, but direct observations are still tenuous and difficult to conclusively interpret. In this study, using Magnetospheric Multiscale (MMS) observations, we
Terry Z. Liu +4 more
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Astronomy and Astrophysics, 2010 Summary: Context. Shocks produced by outflows from young stars are often observed as bow-shaped structures in which the \(H_{2}\) line strength and morphology are characteristic of the physical and chemical environments and the velocity of the impact. Aims.
Gustafsson, Maiken +5 more
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Formation of the bow shock indentation: MHD simulation results
Earth and Planetary Physics, 2021 Simulation results from a global magnetohydrodynamic (MHD) model are used to examine whether the bow shock has an indentation and characterize its formation conditions, as well as its physical mechanism.
BaoHang Qu +5 more
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Geophysical Research Letters, 2023 The Martian bow shock stands as the first defense against the solar wind and shapes the Martian magnetosphere. Previous studies showed the correlation between the Martian bow shock location and solar wind parameters.
Long Cheng +23 more
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To see or not to see a bow shock [PDF]
Astronomy & Astrophysics, 2005 OB-stars have the highest luminosities and strongest stellar winds of all stars, which enables them to interact strongly with their surrounding ISM, thus creating bow shocks. These offer us an ideal opportunity to learn more about the ISM. They were first detected and analysed around runaway OB-stars using the IRAS allsky survey by van Buren et al ...
Brown, D, Bomans, DJ
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