Carbon clusters as a source of C, C2, C3 and their ions in the atmospheres of Comets Giacobini-Zinner and Halley

Details Carbon clusters as a source of C, C2, C3 and their ions in the atmospheres of Comets Giacobini-Zinner and Halley Carbon clusters as a source of C, C2, C3 and their ions in the atmospheres of Comets Giacobini-Zinner and Halley

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.250c.437o&link_type=abstract

In ESA, Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 3: Posters p 437-440 (SEE N87-26714

Physics

1

Carbon, Clumps, Cometary Atmospheres, Giacobini-Zinner Comet, Halley'S Comet, Ionopause, Abundance, Atmospheric Chemistry, Carbon Isotopes, Giotto Mission, International Sun Earth Explorer 3, Vega Project

Scientific paper

The encounters of spacecraft with comets Giacobini-Zinner and Halley
have shown anomalously high relative abundances of
C2+ and C+ respectively. This paper
draws attention to the possibility that carbon clusters may be important
in the production of these anomalies.

Affiliated with

Also associated with

No associations

Rating

Carbon clusters as a source of C, C2, C3 and their ions in the atmospheres of Comets Giacobini-Zinner and Halley does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Carbon clusters as a source of C, C2, C3 and their ions in the atmospheres of Comets Giacobini-Zinner and Halley, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Carbon clusters as a source of C, C2, C3 and their ions in the atmospheres of Comets Giacobini-Zinner and Halley will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1123477