H2O(+) structures in the inner plasma tail of comet Austin

Details H2O(+) structures in the inner plasma tail of comet Austin H2O(+) structures in the inner plasma tail of comet Austin

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acm..proc..257j&link_type=abstract

In Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991 p 257-260 (SEE N93-19113 06-90)

Physics

Austin Comet, Comet Nuclei, Comet Tails, Interplanetary Dust, Plasmas (Physics), Water, Charge Coupled Devices, Continuums, Fabry-Perot Interferometers, Spatial Distribution

Scientific paper

We present images of comet Austin 1989c1 in the light of H2O(+) from
which the contribution of the dust continuum and the gas coma was
completely removed. We describe the behavior of the H2O(+) plasma in the
inner coma where it is reliably observed for the first time.

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