Dust Observations of Comet p/ Halley by the Plasma Wave Analyser

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

This paper reports the electric field observations made with the high-frequency plasma-wave analyser, during the Vega spacecraft encounters with comet Halley on 1986, March 6 and 9. Electric fields are measured in the bandwidth 0-300 kHz with an antenna made of two spheres separated by a distance of 11 m. As the nucleus is approached, the average amplitude and bandwidth of the AC electric field increase dramatically; at frequencies above 1 kHz, the power law index of the electric field spectrum is about - 3.4 (E2 ˜ ƒ-3.4), a value close to those reported elsewhere for random electric pulses induced by dust particles. Moreover, a strong correlation is found between spikes in the quasi-static electric field and small-scale variations in dust count rates for masses less than 10-12 g. Finally we identify several large scale gradients in the AC electric field intensity within 140,000 km from the nucleus which are believed to be associated with enhancements of dust jet activity. The locations of these gradients are used to estimate the apparent rotation period of the cometary nucleus and the radial velocity of the small dust particles.

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