Planetary Atmospheres | ISBN 9789401030656

Planetary Atmospheres

herausgegeben von C. Sagan, Tobias Owen und H.J. Smith
Mitwirkende
Herausgegeben vonC. Sagan
Herausgegeben vonTobias Owen
Herausgegeben vonH.J. Smith
Buchcover Planetary Atmospheres  | EAN 9789401030656 | ISBN 94-010-3065-0 | ISBN 978-94-010-3065-6

Planetary Atmospheres

herausgegeben von C. Sagan, Tobias Owen und H.J. Smith
Mitwirkende
Herausgegeben vonC. Sagan
Herausgegeben vonTobias Owen
Herausgegeben vonH.J. Smith

Inhaltsverzeichnis

  • I / Venus.
  • The chemical composition of the atmosphere of Venus.
  • Exospheric temperature of Venus from Mariner 5.
  • Models of the Venus ionosphere.
  • Venus: Determination of atmospheric parameters from the microwave spectrum.
  • Peculiarities of mm and cm radiowave propagation in the Venus atmosphere.
  • Some consequences of critical refraction in the Venus atmosphere.
  • A two-parameter theory for Venus spectra.
  • A new short-wavelength carbon dioxide band in the spectrum of Venus.
  • Calculations of CO2 energy levels: The Ã1B2 state.
  • High spectral resolution interferometric planetary observations in the 7–25 ? region.
  • Limb darkening observations of Venus from 5 ? to 18 ?.
  • Water on Venus?.
  • Vegetative life on Venus ? Or investigations with algae which grow under pure CO2 in hot acid media and at elevated pressures.
  • Venus cloud contrasts.
  • On the nature of the Venus clouds.
  • Geochemical problems in the production of the Venus clouds.
  • The trouble with Venus.
  • II / Mars.
  • A. Optical Properties.
  • Colorimetry of Martian features by means of area scanning.
  • Longitudinal variations, the opposition effect, and monochromatic albedos for Mars.
  • Mie scattering and the Martian atmosphere.
  • The contribution of atmospheric aerosols to the Martian opposition effect.
  • Ultraviolet polarization measurements of Mars and the opacity of the Martian atmosphere.
  • Some problems of anisotropic scattering in planetary atmospheres.
  • B. CO2 Absorption.
  • An interpretation of the Mars spectrum taken by the Connes.
  • Observations of the Martian 1.2 ? CO2 bands.
  • Variations of the Martian CO2 abundance with Martian season.
  • Relative elevation differences revealed by near infrared CO2 bands on Mars.
  • Spectroscopic determination of surface pressure and elevation differences on Mars.
  • C. Water VaporAbsorption.
  • The spectroscopic search for water on Mars: A history.
  • The latitude variation of water vapor on Mars.
  • A report on Martian atmospheric water vapor near opposition, 1969.
  • High altitude interferometer spectra of Mars.
  • Mars: Occurrence of liquid water.
  • D. Mariner Results.
  • Mariner 6: Ultraviolet spectrum of Mars upper atmosphere.
  • Mariner Mars ’69 celestial mechanics experiment.
  • Mariner 1969: Results of the infrared radiometer experiment.
  • Mariner 6 and 7 television pictures: Preliminary analysis.
  • E. Cloud Motions and Atmospheric Dynamics.
  • Estimates of boundary layer parameters in the atmospheres of the terrestrial planets.
  • The theory of similarity for large-scale motions in planetary atmospheres.
  • Cloud activity on Mars near the equinox: Comparison of the 1937 and 1969 oppositions.
  • Cloud motions on Mars.
  • F. Upper Atmospheres.
  • The effect of atmospheric dynamics on the upper atmosphere phenomena of Mars and Venus.
  • CO2+ dayglow on Mars and Venus.
  • III / Outer Planets.
  • Variations in the color of Jupiter.
  • The effective temperature of Jupiter’s equatorial belt during the 1965 apparition.
  • Observations of Jupiter’s cloud structure near 8.5 ?.
  • Phase behavior of light gas mixtures at high pressures.
  • Atmospheric depths of Jupiter, Saturn, and Uranus.
  • The spectral characteristics and probable structure of the cloud layer of Saturn.
  • Estimate of the H2 abundance in the atmosphere of Uranus from the pressure induced spectrum.
  • The spectrum of Uranus in the region 4800–7500 Å.
  • Upper limit of hydrogen and helium concentrations on Titan.
  • IV / Scientific Dedication of the 107-Inch Reflector.
  • Remarks made at the scientific dedication of the 107-inch reflector, October 30, 1969.