Bow shock (aerodynamics)
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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Simulation study of magnetic holes at the Earth's collisionless bow shock
... hand side of the simulation box, and the downstream side is assumed to be on the left-hand side, and the simulation box is assumed to be in the frame of the bulk plasma of the solar wind. In the centre of the simulation ...
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Interstellar Medium Parameters in Front of the External Bow Shock
... the shock front are well-determined by the known laws and ...external bow shock contain much information about physical parameters ahead of the external bow shock front (about ...
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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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Acceleration of solar wind ions to 1 MeV by electromagnetic structures upstream of the Earth's bow shock
... Magnetic pulsations described above represent typical foreshock phenomena, called also SLAMS [17], and have been associated with ion-ion right-hand resonant instabil- ity [18,19]. According to this model, the instability ...
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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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The IMF control of the Martian bow shock and plasma flow in the magnetosheath Predictions of 3 D simulations and observations
... of shock dis- tances, which can be as large as 10%, is a consequence of the varying speed of propagation of fast magnetosound waves (Cloutier, 1976; Romanov, 1978; Russell et ...venusian bow shock at ...
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Low frequency magnetic variations at the high β Earth bow shock
... Earth’s bow shock during high-β (ratio of thermal to magnetic pressure) solar wind streams are ...the shock transition have am- plitudes much larger than the background field and have a frequency of ...
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Large amplitude solitary waves in and near the Earth’s magnetosphere, magnetopause and bow shock: Polar and Cluster observations
... Solitary waves have been identified throughout the Earth’s magnetosphere at narrow boundaries, such as the plasma sheet boundary (Matsumoto et al., 1994; Franz et al., 1998; Cattell et al., 1999) and the bow ...
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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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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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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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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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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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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 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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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 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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