Electron-density distribution in Comet Halley according to radio-sounding data

Details Electron-density distribution in Comet Halley according to radio-sounding data Electron-density distribution in Comet Halley according to radio-sounding data

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kosis..28..293a&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 28, Mar.-Apr. 1990, p. 293-303. In Russian.

Computer Science

Sound

1

Density Distribution, Electron Density (Concentration), Halley'S Comet, Radio Probing, Satellite Sounding, Coherent Radiation, Electron Density Profiles, Radio Signals, Venera Satellites

Scientific paper

The electron density profile as a function of cometocentric distance, N(h), was constructed for Comet Halley on the basis of the sounding of the comet's shell by coherent radio signals from the Vega 1 and 2 probes. A local peak of electron density is observed at a cometocentric distance of (11.5 + or - 0.5) x 10 to the 3rd km. The electron density distribution of the cometary plasma in the range of cometocentric distances from 11.5 x 10 to the 3rd to 5 x 10 to the 4th km can be represented as N(h) approximately equal to h exp -2.

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