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  • 1
    Publication Date: 2011-08-19
    Description: Preliminary results from electric field measurements in the environment of Mars using the plasma-wave system on board Phobos 2 are reported. Electron-plasma oscillations observed upstream of the bow shock correspond to a solar-wind density of 2/cu cm. The shock-foot boundary was crossed up to three times on each orbit. The shock ramp was detected at altitudes between 0.45 and 0.75 Mars radii R(M) above the planetary surface. The density increased by about a factor of two at the ramp. The shock position, although variable, seems to be consistent with previous measurements. The downstream magnetosheath contained broadband electric-field noise below the plasma frequency. The boundary of th obstacle, or plasmapause, was crossed at altitudes of the order of 0.28 R(M); the cold plasma density was highly variable within the planetopause and reached the unexpected value of 700/cu cm on the third orbit, at 0.25 R(M) altitude. Bursts of waves with frequencies below the electron cyclotron frequency occur within the planetopause.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Nature (ISSN 0028-0836); 341; 607-609
    Format: text
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  • 2
    ISSN: 1572-9486
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The paper discusses the dynamics of solar wind proton,α-particle and electron fluxes near the Earth's bow shock front. In subsequently developed events, deceleration and deflection of ion components and electron heating are observed. The velocity distributions of protons andα-particles behind the shock front have a strongly inhomogeneous structure that is gradually smoothing out in the magnetosheath. Unlike protons,α-particles behind the front do not generate beams with energy exceeding that of the solar wind.
    Type of Medium: Electronic Resource
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