Electrodynamics of submicron dust in the cometary coma

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Comet Heads, Comet Nuclei, Cosmic Dust, Electric Charge, Electrodynamics, Halley'S Comet, Cometary Atmospheres, Electric Potential, Electromagnetic Shielding, Giotto Mission, Secondary Emission, Solar Wind Velocity, Spacecraft Shielding, Vega Project, Comets, Comae, Electromagnetic Effects, Dust, Solar Wind, Grains, Size, Composition, Plasmas, Radiation, Pressure, Accelerations, Charged Particles, Giotto Mission, Vega Mission, Electrodynamics

Scientific paper

Electromagnetic forces derived from the solar wind fields act strongly on submicron dust grains in the cometary coma. The grain charge and thus the forces are sensitive to composition and cometary plasma conditions, as well as to grain size. For dielectric grains of 0.1 μm and conducting grains of 0.3 μm or less, the electromagnetic forces dominate over radiation pressure. The stronger accelerations may produce fan-like structures as sometimes observed. They would also cause grains to circumvent the shields designed to protect the Giotto and Vega spacecrafts speeding through comet Halley's dust coma.

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