Scalar-potential mapping of the steady-state magnetosheath model [PDF]
Annales GeophysicaeThe steady-state magnetosheath model has various applications for studying the plasma and magnetic field profile around the planetary magnetospheres.
Y. Narita, D. Schmid, S. Toepfer
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Asymmetries in the Earth's dayside magnetosheath: results from global hybrid-Vlasov simulations [PDF]
Annales Geophysicae, 2020 Bounded by the bow shock and the magnetopause, the magnetosheath forms the interface between solar wind and magnetospheric plasmas and regulates solar wind–magnetosphere coupling.
L. Turc +10 more
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South-north asymmetry of proton density distribution in the Martian magnetosheath
Earth and Planetary Physics, 2020 We perform a statistical analysis of data from the Mars Atmosphere and Volatile Evolution (MAVEN) project on the global distribution of protons in the Martian magnetosheath.
Jing Wang +3 more
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Magnetosheath cavities: case studies using Cluster observations [PDF]
Annales Geophysicae, 2009 This paper presents examples of magnetosheath cavities in Cluster spacecraft observations. The cavities are accompanied by high energy particles in the magnetosheath and characterized by depressed magnetic fields and densities.
F. T. Katırcıoğlu +5 more
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Plasma and Magnetic Field Turbulence in the Earth’s Magnetosheath at Ion Scales [PDF]
Frontiers in Astronomy and Space Sciences, 2021 Crossing the Earth’s bow shock is known to crucially affect solar wind plasma including changes in turbulent cascade. The present review summarizes results of more than 15 years of experimental exploration into magnetosheath turbulence.
Liudmila Rakhmanova +2 more
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Magnetosheath waves under very low solar wind dynamic pressure: Wind/Geotail observations [PDF]
Annales Geophysicae, 2005 The expanded bow shock on and around "the day the solar wind almost disappeared" (11 May 1999) allowed the Geotail spacecraft to make a practically uninterrupted 54-h-long magnetosheath pass near dusk (16:30-21:11 magnetic local time) at a radial ...
C. J. Farrugia +10 more
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Magnetosheath Jets Over Solar Cycle 24: An Empirical Model. [PDF]
J Geophys Res Space Phys, 2023 Vuorinen L +3 more
europepmc +3 more sources
Reflection and Refraction of the L-O Mode 5 kHz Saturn Narrowband Emission by the Magnetosheath. [PDF]
Geophys Res Lett, 2022 Wu SY +7 more
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The Earth's magnetosheath: Structures, waves and turbulence
地球与行星物理论评, 2022 When the solar wind encounters the blunt Earth's magnetosphere, a detached shock (i.e., the bow shock) forms at a distance about ten Earth radii from the Earth.
Shiyong Huang
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Magnetosheath plasma flow model around Mercury [PDF]
Annales Geophysicae, 2021 The magnetosheath is defined as the plasma region between the bow shock, where the super-magnetosonic solar wind plasma is decelerated and heated, and the outer boundary of the intrinsic planetary magnetic field, the so-called magnetopause.
D. Schmid +5 more
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