The Visual and Near-Infrared Spectrum of Methane and its Application to Uranus, Neptune, Triton and Pluto.

The machine has a rotatable material pickup device movably supported on a portable frame for movement relative to the rear end of the frame to a lowered material pickup position and to an elevated position wherein a formed bale can pass thereunder. A pair of fixed vertically spaced rollers are located forwardly of the pickup device. A third roller is movable longitudinally of the frame in a path above and to opposite sides of the upper one of the rollers and is continuously yieldably urged in a direction toward the front end of the frame. A continuous belt means is initially trained about the pickup device, the bottom fixed roller and the movable roller, with the lower run of the belt means, extended between the pickup device and the bottom fixed roller, lying in a substantially horizontal plane adjacent the ground surface. As the portable frame is advanced along a windrow, the material gathered by the pickup device is engaged by the lower run of the belt means for compaction and rolling on the ground surface. During a bale forming operation the belt lower run is progressively extended about the bale concurrently with the rearward movement of the third roller to train the flexible means about the upper fixed roller. On completion of the bale, the pickup device is elevated and the frame moved away from the ground supported bale.

[1]  L. Wallace The structure of the Uranus atmosphere , 1980 .

[2]  D. McClure,et al.  The vibrational overtone spectrum of liquid methane in the visible and near infrared - Applications to planetary studies , 1978 .

[3]  W. Cochran,et al.  Raman scattering in the atmospheres of the major planets , 1978 .

[4]  U. Fink,et al.  Band model analysis of laboratory methane absorption spectra from 4500 to 10500 A , 1977 .

[5]  R. E. Danielson The structure of the atmosphere of Uranus , 1977 .

[6]  G. R. Smith,et al.  The interpretation of Jovian methane absorptions. , 1977 .

[7]  D. Morrison,et al.  Pluto: Evidence for Methane Frost , 1976 .

[8]  M. J. Price,et al.  Limb brightening on Uranus - The visible spectrum , 1976 .

[9]  T. Owen,et al.  On the 6825 A band of methane , 1976 .

[10]  L. Trafton The aerosol distribution in Uranus' atmosphere - Interpretation of the hydrogen spectrum , 1976 .

[11]  T. Owen,et al.  Laboratory band strengths of methane and their application to the atmospheres of Jupiter, Saturn, Uranus, Neptune, and Titan , 1976 .

[12]  L. Wallace On the thermal structure of Uranus , 1975 .

[13]  R. Cess,et al.  Methane absorption in the visible spectra of the outer planets and Titan , 1975 .

[14]  M. Belton,et al.  An estimate of the temperature and abundance of CH4 and other molecules in the atmosphere of Uranus , 1975 .

[15]  M. Belton,et al.  Why image Uranus , 1975 .

[16]  R. E. Danielson The Visible Spectrum of Uranus , 1974 .

[17]  C. Porco,et al.  On the identification of the 6420 A absorption feature in the spectra of Uranus and Neptune , 1974 .

[18]  M. H. Hart A possible atmosphere for Pluto , 1974 .

[19]  JOHN S. Lewis,et al.  Atmospheric and cloud structures of the Jovian planets , 1973 .

[20]  J. Margolis,et al.  The temperature dependence of the half widths of some self-and foreign-gas-broadened lines of methane , 1973 .

[21]  M. J. Price,et al.  Observation of the Raman Effect in the Spectrum of Uranus , 1973 .

[22]  A. Cameron,et al.  Abundances of the elements in the solar system , 1973 .

[23]  B. Lutz Molecular Hydrogen on Uranus: Observation of the 3-0 Quadrupole Band , 1973 .

[24]  M. J. Price The scattering mean free path in the Uranian atmosphere , 1973 .

[25]  W. Sinton Limb and polar brightening of Uranus at 8870 A. , 1972 .

[26]  B. Lutz,et al.  New observations on the Kuiper bands of Uranus. , 1972 .

[27]  T. C. Flandern,et al.  The Diameter of Neptune , 1969 .

[28]  R. E. Danielson,et al.  A Two-Layer Model of the Jovian Clouds , 1969 .

[29]  J. Hansen Radiative transfer by doubling very thin layers , 1969 .

[30]  L. Trafton Model atmospheres of the major planets , 1967 .

[31]  T. Owen An Identification of the 6800-Å Methane Band in the Spectrum of Uranus and a Determination of Atmospheric Temperature , 1966 .

[32]  T. Mullikin,et al.  CHANDRASEKHAR'S X- AND Y- FUNCTIONS, , 1966 .

[33]  U. Oppenheim,et al.  Emissivity of Water Vapor at 1200°K in the 1.9- and 2.7-µ Regions* , 1965 .

[34]  H. Mayer Opacity calculations, past and future , 1964 .

[35]  H. Spinrad Pressure-Induced Dipole Lines of Molecular Hydrogen in the Spectra of Uranus and Neptune. , 1963 .

[36]  H. Crosswhite,et al.  New Spectrometer Slit Mechanism , 1956 .

[37]  William G. Fastie,et al.  A Small Plane Grating Monochromator , 1952 .

[38]  Gerard P. Kuiper,et al.  Titan: a Satellite with an Atmosphere. , 1944 .

[39]  John U. White Long Optical Paths of Large Aperture , 1942 .

[40]  T. Martin Saturn and Jupiter : a study of atmospheric constituents , 1975 .

[41]  T. Encrenaz,et al.  Observational Constraints on Model Atmospheres for Uranus and Neptune , 1974 .

[42]  JOHN S. Lewis,et al.  Uranus atmosphere - Structure and composition. , 1973 .

[43]  D. Mccarthy,et al.  The infrared spectral albedo of Uranus , 1972 .

[44]  J. Poll ESTIMATE OF THE H2 ABUNDANCE IN THE ATMOSPHERE OF URANUS FROM THE PRESSURE INDUCED SPECTRUM , 1971 .

[45]  H. Spinrad,et al.  Molecular Hydrogen Features in the Spectra of Saturn and Uranus , 1966 .

[46]  H. Mayer Methods of Opacity Calculations , 1949 .