Bow Shock
Electrostatic quasi monochromatic waves in the downstream region of the Earth’s bow shock based on Geotail observations
... Shin et al. (2005) reported that EQM waves are accom- panied by electron beam-like components. Figure 2 shows the electron velocity distribution observed by the low en- ergy particle (LEP) experiment (Mukai et al., 1994) ...
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Acceleration of solar wind ions to 1 MeV by electromagnetic structures upstream of the Earth's bow shock
... by shock waves ...planetary bow shocks, and at bound- aries between streams of fast and slow solar wind plasma in co-rotating interaction regions ...Earth’s bow shock [5] is generally ...
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Simulation study of magnetic holes at the Earth's collisionless bow shock
... Earth’s bow shock [2], and foreshock cavities observed by the Wind satellite ...Earth’s bow shock, the Cluster and Double Star satellites have recently recorded density and magnetic holes with ...
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The IMF control of the Martian bow shock and plasma flow in the magnetosheath Predictions of 3 D simulations and observations
... observed bow shock does not contain a “bulge” in the direction opposite to the direction of the motional electric field, which was pre- dicted by the 3D hybrid simulations, note that planetary ions were not ...
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Jump conditions for pressure anisotropy and comparison with the Earth’s bow shock
... the shock, one has to use an additional equation, since the set of equations is un- ...the bow shock and the magnetopause, might be taken into ac- ...
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Kis, Arpad (2005): Energetic Ions at Earth's Quasi-Parallel Bow Shock. Dissertation, LMU München: Fakultät für Geowissenschaften
... the bow shock (Ipavich et ...the bow shock (Forman and Drury, ...the shock drift acceleration contributes to the energization ...
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Interstellar Medium Parameters in Front of the External Bow Shock
... external bow shock is given, as well as the form of ...external bow shock are paraboloids of rotation and differ only in various distances to the nose ...external bow shock front ...
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Large amplitude solitary waves in and near the Earth’s magnetosphere, magnetopause and bow shock: Polar and Cluster observations
... The data for the Cluster study were obtained as the Clus- ter satellites traversed the bow shock, magnetopause, cusp and the plasma sheet boundary. The electric field and space- craft potential measurements ...
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Wind observations of the terrestrial bow shock: 3 D shape and motion
... eled bow shock along the same direction ...tary shock was crossed at 15.40 on May 5 that resulted in bow shock moving towards the Earth from the spacecraft and thus it was passed by the ...
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Low frequency magnetic variations at the high β Earth bow shock
... bow shock. For example, in a supercritical quasi-perpendicular shock, the oblique whistler waves near the lower-hybrid frequency (∼ 5 Hz) form the magnetic ramp via the nonlinear steepening and decay ...
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Wavelet application to the magnetic field turbulence in the upstream region of the Martian bow shock
... In this paper, we compare magnetic field fluctuations with the observations of backstreaming ions. One should keep in mind that Phobos-2 data about the ions streaming in a sunward direction are rather scarce. The ASPERA ...
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On the vorticity behind 3-D detached bow shock wave
... For the general case of a spatial isoenergetic flow of ideal gas, Helmholtz ’ s theorems are generalized and the speed with which vortex tubes move is found, keeping the intensity. It is shown that along the streamline ...
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Statistical survey of day side magnetospheric current flow using Cluster observations: bow shock
... Dunlop et al. (2001) pointed out that high-frequency fluc- tuations are likely to cause uncertainties within the curlome- ter results and suggest an appropriate averaging in time be- fore applying the curlometer to ...
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Ion and electron heating at the Martian bow shock Common for bow shocks or not?
... the bow shock exists near Mars (Riedler et ...subsolar bow shock, and evaluated that about 30% of solar wind protons might be reflected at the electrostatic barrier of the ...Mars’s bow ...
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Dispersion of low frequency plasma waves upstream of the quasi-perpendicular terrestrial bow shock
... the shock front ...internal shock dy- namics resulting in quasi-periodic steepening and overturn- ing of the shock front ...the shock front has been considered to be the result of two stream ...
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Numerical investigation of an active TPS for a wing leading edge exposed to high temperature air behind a strong bow shock wave
... the bow shock wave formed in front of the cylinder is nearly perfectly blocked by the coolant gas issuing from around the stagnation point despite the occurrence of the Kelvin-Helmholtz instability, which ...
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The Martian bow shock over solar cycle 23 24 as observed by the Mars Express mission
... Between the solar minimum and maximum phases of cycle 23-24, the average Martian bow shock distance increases by 7% 2.. The bow shock surface is modeled from Mars Express observations ov[r] ...
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Reflection of the strahl within the foot of the Earth's bow shock
... one then expects to see a bimodal density pattern. High den- sity implies that the spacecraft is located in the foreshock and is seeing reflected electrons. Low density indicates that the spacecraft is located in the ...
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Ion acceleration by multiple reflections at Martian bow shock
... have not been observed for the terrestrial bow shock. Recently, the Mars Express (MEX) Ion Mass Analyzer (IMA) has detected accelerated ions at multiple discrete energies (at least three energies) above the ...
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The IMF bending upstream of the Martian bow shock
... Dubinin et al.(1995) have supposed that a sudden rotation of the magnetic field across the foreshock boundary might be associated with a current of reflected pickup protons. Using a simple model based on test particle ...
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