Physics
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989natur.341..607g&link_type=abstract
Nature (ISSN 0028-0836), vol. 341, Oct. 19, 1989, p. 607-609. Research supported by NASA.
Physics
63
Magnetosheath, Mars Environment, Mars Probes, Planetary Magnetic Fields, Plasma Waves, Satellite Observation, Electron Plasma, Electrostatic Probes, Solar Planetary Interactions, Soviet Spacecraft
Scientific paper
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.
Grard Rejean
Klimov Stanislav
Pedersen Andreas
Savin Sergei
Skalskii A. A.
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