Physics
Scientific paper
Apr 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988rpsct...5...19g&link_type=abstract
In its JPRS Report: Science and Technology. USSR: Space p 19-20 (SEE N88-20312 13-12) Transl. into ENGLISH from Kosmicheskiye Is
Physics
Halley'S Comet, Hydrocarbons, Infrared Radiation, Infrared Spectroscopy, Spectral Bands, Spectrum Analysis, Vega Project, Molecules, Solar Radiation, Spacecraft Instruments
Scientific paper
The 3.35 micron hydrocarbon band is analyzed on the assumption that the emitting matter is in a gaseous state and the excitation source is solar ultraviolet radiation. The analysis method is described and qualitative estimates are given. The band was first broken down into three distinctive regions (3.22 to 3.25, 3.31 to 3.42 and 3.45 to 3.51 microns), corresponding to vibrations of different groups of atoms. Each of these three regions is analyzed in detail.
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