Computer Science
Scientific paper
Apr 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icar...42...93s&link_type=abstract
Icarus, vol. 42, Apr. 1980, p. 93-101.
Computer Science
4
Ammonia, Jupiter Atmosphere, Saturn Atmosphere, Abundance, Atmospheric Models, Telescopes, Planets, Saturn, Jupiter, Atmosphere, Ammonia, Abundance, Models, Data, Hydrogen, Element Ratios, Absorption, Pressure, Observations, Thickness, Theoretical Studies, Wavelengths, Bandwidths, Thermal Structure, Spectrum, Temperatures, Layers, Reflectance, Scattering, Optical Properties, Clouds
Scientific paper
A profile and equivalent width for the 6451.1-A feature of the 6450-A band of ammonia at the equator and south pole of Saturn have been measured. Estimates for the NH3 abundance at the center of the disk which vary from 0.4 to 5 m-am, depending upon the atmospheric model used, lead to uncertainties in the NH3/H2 ratio which are greater than a factor of 10. Half-widths for theoretical line profiles computed from models in which the NH3 absorption occurs at a pressure level of 1.0 atm agree with the observed profiles. NH3/H2 ratios have been obtained which range from 0.00001 to 0.00002 for Jupiter.
Cochran William D.
Macy William W.
Smith William Hayden
No associations
LandOfFree
Ammonia in the atmospheres of Saturn and Jupiter 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 Ammonia in the atmospheres of Saturn and Jupiter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ammonia in the atmospheres of Saturn and Jupiter will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1698942