Plasma and waves around Mars

Astronomy and Astrophysics – Astronomy

Scientific paper

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Energy Spectra, Mars Probes, Onboard Equipment, Phobos, Plasma Waves, Electron Plasma, Plasma Density, Solar Wind, Spaceborne Astronomy, Mars, Plasma Waves, Pws Instrument, Spacecraft Observations, Electrons, Phobos 2 Mission, Density, Electrical Field, Oscillations, Upstream, Bow Shock, Solar Wind, Magnetosheath, Magnetopause, Altitude, Spectra, Electromagnetic Waves, Frequencies, Emissions, Electrostatic Effects, Atmosphere, Diagrams, Boundaries, Comparisons

Scientific paper

The Plasma Wave System (PWS) onboard the Phobos 2 collected data which revealed the high variability of the Martian environment in the sunward hemisphere during successive orbits. The PWS recorded the spectra of natural waves and measured the plasma density distribution using a Langmuir probe. Measurements are based on data collected around the periapsis of the first four orbits around Mars. Electron plasma oscillations are observed upstream of the bow shock and the shock foot and/or ion foreshock are detected on each orbit. The downstream solar wind, in the planetosheath, is characterized by increased plasma density and broadband electrostatic noise. A comparison between the times of the bow shock and planetopause crossings observed with various instruments is given.

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