Results 21 to 30 of about 2,940 (168)
3D simulations of Betelgeuse’s bow shock [PDF]
Minor revisions, replaced Fig. 1, 15, and 16, added movies.
Mohamed, S., Mackey, J., Langer, N.
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Bow shock motions observed with CLUSTER [PDF]
The Cluster mission allows the determination not only of the bow shock crossing position but also, with a simple timing method and a reasonable confidence, the shock normal and the velocity along this normal. We apply this technique to a series of eleven consecutive bow shock crossings which occurred during a time interval of approximatively two and a ...
Maksimovic, Milan +3 more
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Pulsar bow-shock nebulae [PDF]
17 pages, Latex, 6 Encapsulated PostScript figures, accepted for publication in A& ...
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review paper on current state of knowledge about planetary bow shocks, 32 pp, 19 ...
Treumann, R. A., Jaroschek, C. H.
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Variability of Bow Shock Location at Mars [PDF]
Bow shock formation, in case the supersonic solar wind flow is hindered by the atmosphere of Mars, is investigated. The atoms newly ionized from the extensive neutral atmosphere of Mars are loaded to the solar wind.
Yu Yi, Eojin Kim, Yong Ha Kim, Jhoon Kim
doaj
Reflection of the strahl within the foot of the Earth's bow shock [PDF]
The reflection of a fraction of the solar wind at the bow shock to some extent defines the physical properties of what is known as the foreshock, the region where the interplanetary magnetic field has a direct connection to the bow shock.
C. A. Gurgiolo +3 more
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A model of the magnetosheath magnetic field during magnetic clouds [PDF]
Magnetic clouds (MCs) are huge interplanetary structures which originate from the Sun and have a paramount importance in driving magnetospheric storms. Before reaching the magnetosphere, MCs interact with the Earth's bow shock.
L. Turc +3 more
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Multispacecraft observations of the terrestrial bow shock and magnetopause during extreme solar wind disturbances [PDF]
Three events are discussed from the declining phase of the last solar cycle when the magnetopause and/or the bow shock were observed unusually close to the Earth due to major interplanetary disturbances.
M. Tátrallyay +4 more
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We have used the AMR-CESE-MHD model to investigate the influences of the IMF Bz and the upstream solar wind dynamic pressure (Dp) on Earth’s magnetopause and bow shock.
Wang Juan +5 more
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Properties and the origin of Almost Monoenergetic Ion (AMI) beams observed near the Earth's bow shock [PDF]
Beams of Almost Monoenergetic Ions (AMI) in the energy range from 20 to 800 keV were discovered in the DOK-2 experiment (Interball project) in the magnetosheath and upstream of the Earth's bow shock.
V. N. Lutsenko, E. A. Gavrilova
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