Numerical simulation of surface brightness distribution in the ion tail of the Comet ‘/1976 R1 (West)

Details Numerical simulation of surface brightness distribution in the ion tail of the Comet ‘/1976 R1 (West) Numerical simulation of surface brightness distribution in the ion tail of the Comet ‘/1976 R1 (West)

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002kfnt...18..128s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 18, no. 2, p. 128-135

Computer Science

Scientific paper

Surface photometry of the comet ‘/1976 R1( West) plates was carried out. The surface brightness distribution in the streams in the ion tail of the comet is compared to model calculations. The diffusion model of ion tails was used in the calculations. The upper limits of the lifetime of luminous particles and the magnetic field induction in the tail and the lower limits of the diffusion coefficients are estimated.

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