Other
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.250a.311w&link_type=abstract
In ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 1: Plasma and Gas p 311-316 (SEE N87
Other
8
Abundance, Emission Spectra, Halley'S Comet, Molecular Ions, Molecular Spectroscopy, Space Plasmas, Astronomical Spectroscopy, Carbon Dioxide, Comet Tails, Ion Emission
Scientific paper
Spectroscopic observations (4000 - 7000 Å) were obtained of comet P/Halley near the time of the spacecraft encounters in March 1986. New molecular ion emission features were observed in the long-slit CCD spectra. Additional spectroscopic observations obtained in April 1986 confirm the presence of many new ion features in the plasma tail. Here the authors propose that CO2+ be identified with the new features in the 4000 - 4350 Å region. The authors suggest that the other unidentified ion features may be attributable to a single ion species.
Belton Michael J. S.
Spinrad Hyron
Wehinger Peter A.
Wyckoff Susan
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