Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.250a.465k&link_type=abstract
In ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 1: Plasma and Gas p 465-469 (SEE N87
Astronomy and Astrophysics
Astronomy
2
Emission Spectra, Halley'S Comet, Hydroxyl Radicals, Line Spectra, Water, Astronomical Models, Iue, Parameter Identification, Vega Project
Scientific paper
Curves of growth of emission lines are calculated for both parent and secondary species with Haser model of comet. Variations of these curves when varying input parameters are discussed. The technique developed is applied to the measurements of H2O 2.7 and 1.38 μm bands by the Vega spacecraft and to OH 3090 Å band measured by Vega 2 and IUE. Evaluation of the H2O total production rate of 1030s-1 at March 9, 1986 obtained by this technique should be considered as the lower limit and the real value may be a factor of 1.5 - 2 over due to H2O ejection in sunward direction.
Krasnopolsky Vladimir A.
Tkachuk Yu. A.
No associations
LandOfFree
Curves of growth of emission lines in cometary spectra: Implications to H2O and OH bands of Comet 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 Curves of growth of emission lines in cometary spectra: Implications to H2O and OH bands of Comet Halley, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Curves of growth of emission lines in cometary spectra: Implications to H2O and OH bands of Comet Halley will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1122559