Results 31 to 40 of about 116,603 (307)
Pulsar bow-shock nebulae [PDF]
Astronomy & Astrophysics, 2002 17 pages, Latex, 6 Encapsulated PostScript figures, accepted for publication in A& ...
openaire +2 more sources
, 2008 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]
Journal of Astronomy and Space Sciences, 1999 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]
Annales Geophysicae, 2019 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]
Annales Geophysicae, 2014 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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Models of the circumstellar medium of evolving, massive runaway stars moving through the Galactic plane [PDF]
, 2014 At least 5 per cent of the massive stars are moving supersonically through the interstellar medium (ISM) and are expected to produce a stellar wind bow shock.
Gvaramadze, V. V. +6 more
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Properties and the origin of Almost Monoenergetic Ion (AMI) beams observed near the Earth's bow shock [PDF]
Annales Geophysicae, 2011 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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Bow-shock Pulsar Wind Nebulae Passing Through Density Discontinuities
, 2016 Bow-shock pulsar wind nebulae are a subset of pulsar wind nebulae that form when the pulsar has high velocity due to the natal kick during the supernova explosion.
Heinz, Sebastian, Yoon, Doosoo
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Journal of Space Weather and Space Climate, 2018 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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Multispacecraft observations of the terrestrial bow shock and magnetopause during extreme solar wind disturbances [PDF]
Annales Geophysicae, 2012 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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