Laboratory simulation of absorption spectra in cloudy atmospheres
Laboratory analog simulation of absorption line spectra in cloudy planetary atmospheres, comparing with computational model based on plane parallel atmosphere
Hunt, G. E.↗
Engineering topics
Margolis, J. S.
Publications and source records attributed to Margolis, J. S..
High dispersion spectroscopic studies of Mars. V - A search for oxygen in the atmosphere of Mars.
In order to set a new upper limit on the amount of diatomic oxygen in the atmosphere of Mars, we have reduced a number of high-dispersion spectra of the 7620 A band of oxygen obtained during the 1969 apparition of Mars. Our new upper limit is 15 atm cm(stp) for the Martian abundance in a single vertical path. This result confirms and lowers the 1963 upper limit of 70 cm atm(stp) by Kaplan, Muench, and Spinrad (1964). The features reported by Hunten and Belton (1966) do not appear on our spectra. Further, we have measured the pressure shift of the A band in the laboratory, and found that the shift required by their tentative identification of diatomic oxygen in the Martian atmosphere does not exist. We conclude that their tentative identification was spurious, and their upper limit dubious.
Margolis, J. S.↗
Studies of methane absorption in the Jovian atmosphere. III - The reflecting-layer model
Reflecting layer model for methane band absorption spectrum in Jovian atmosphere
Margolis, J. S.↗
Recomputation of the absorption strengths of the methane 3 nu sub 3 J-manifolds at 9050 cm to the minus 1
Absorption intensities of R branch J manifolds of methane band, using half widths and pressure shifts
Bergstralh, J. T.↗
Self-broadened half-widths and pressure shifts for the R-branch J-manifolds of the 3 nu sub 3 methane band
Methane spectral band analysis, examining J manifolds self broadening coefficients of R branch
Margolis, J. S.↗
Measurement of the absorption strength of the methane 3 nu sub 3, J-manifolds at 9050/cm
Absorption strengths of j-manifolds in R branch of Jupiter atmosphere methane band, discussing fine structure blending
Margolis, J. S.↗
Studies of methane absorption in the Jovian atmosphere. II
Methane abundance in Jovian atmosphere deduced from line equivalent widths, obtaining line intensity for J manifolds
Fox, K.↗
Extension of calculations of rotational temperature and abundance of methane in the Jovian atmosphere
Rotational temperatures and methane abundances in Jovian atmosphere calculated for various Lorentz half widths
Fox, K.↗
Studies of methane absorption in the Jovian atmosphere. I.
Methane rotational temperature in Jovian atmosphere deduced from equivalent widths of lines at 1.1 micron band
Fox, K.↗
Infrared absorption spectrum of CH sub 4 at 9050 cm super - super 1.
Methane IR absorption band centered near wavenumber 9050, noting R branch features and fine structure
Fox, K.↗