Optical and hydrodynamic implications of Comet Halley dust size distribution

Details Optical and hydrodynamic implications of Comet Halley dust size distribution Optical and hydrodynamic implications of Comet Halley dust size distribution

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987esasp.278..399c&link_type=abstract

In ESA, Proceedings of the International Symposium on the Diversity and Similarity of Comets p 399-408 (SEE N88-21884 14-91)

Computer Science

14

Cosmic Dust, Halley'S Comet, Hydrodynamics, Infrared Spectra, Particle Size Distribution, Spectrum Analysis, Deceleration, Giotto Mission, Spatial Distribution, Vega Project

Scientific paper

Using a specially developed radiative hydrodynamic code, the compatibility between the dust fluences recorded by detectors on Giotto and Vega, the rate of deceleration of the Giotto spacecraft encounter, and a set of pre and postperihelion spectra of Halley extending from near to far infrared wavelengths are examined. It is proposed that the average coma dust distribution is well represented by the envelope of those deducible from the fluences of the VEGA and Giotto probes. Implications of this suggestion are quantitatively investigated.

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