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Author:   A. Woszczyk ,  C. Iwaniszewska
Publisher:   Springer
Imprint:   Kluwer Academic Publishers
Edition:   1974 ed.
Volume:   65
Dimensions:   Width: 15.60cm , Height: 3.30cm , Length: 23.40cm
Weight:   0.991kg
ISBN:  

9789027704498

ISBN 10:   902770449
Pages:   577
Publication Date:   31 October 1974
Audience:   General/trade ,  General
Format:   Hardback
Publisher's Status:   Active
Availability:   Temporarily unavailable  
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Table of Contents

I / Origin and General Physics of the Planetary System.- Planetary Formation.- Status of Molecular Opacities of Interest in the Modeling of a Proto-Solar Nebula.- On the Growth Mechanism of Grains in a Primordial Stage of the Solar Nebula.- The Escape of Planetary Atmospheres.- Modern Research in High Resolution Infrared Spectroscopy and Its Importance to Planetary Physics.- Optical Properties of Particles in Planetary Atmospheres: Laboratory Studies.- First Results of the Soviet-Polish Space Experiment ‘Intercosmos-Kopernik 500’.- II / Terrestrial Planets.- Infrared Spectra of Venus.- Radio Interferometry of Venus at Short Wavelengths.- Profondeur de pénétration et formation des raies dans une atmosphère diffusante.- Etude théorique de la répartition de luminance sur le disque de Venus.- Numerical Modelling of the Reflection Spectrum of Venus in the Visual and Near Infrared Ranges.- Interpretation of the Illumination Measurements by the Automatic Interplanetary Station ‘Venera 8’.- Nature of the Venus Clouds as Derived from Their Polarization.- Water Vapor in Venus Determined by Airborne Observations of the 8200 Å Band.- Ground-Based Observations of Mars and Venus Water Vapor during 1972 and 1973.- Observations of O2, H2O and HD in Planetary Atmospheres.- The Spectrum of Mars in the Region 1800–3200 cm?1.- Results of Current Mars Studies at the IAU Planetary Research Center.- UBV Photometry of Mars.- Photometric Data from Some Photographs of Mars Obtained with the Automatic Interplanetary Station ‘Mars 3’.- Results from the Infrared Spectroscopy Experiment on Mariner 9.- Radio Occultation Exploration of Mars.- Mars: Local Structure of Dust Storms.- III / Outer Planets and Their Satellites.- The Hydrogen to Helium Mixing Ratio in the GiantPlanets.- On the Equation of State of Hydrogen and Its Use in Models of Major Planets.- The Influence of the Surface Boundary Layer on Evolutionary Models of Jupiter.- Observations of Spatial and Temporal Variations of the Jovian H2 Quadrupole Lines.- TDIA Satellite Spectroscopic Observations of Jupiter in the Ultraviolet.- New Infrared Spectra of the Jovian Planets: Study of Jupiter and Saturn in the 3v3 Methane Band by Fourier Transform Spectroscopy.- On the Microwave Spectrum of Methane in the Atmospheres of the Outer Planets.- Jupiter’s Microwave Spectrum: Implications for the Upper Atmosphere.- Jupiter’s Radiation Belts and Upper Atmosphere.- Analysis of Spectroscopic Observations of Jupiter and the Variability of the Structure of the Visible Clouds.- Motions in Jupiter’s Atmosphere.- Results of the Beta Scorpii Occultation by Jupiter on May 13, 1971.- Atmospheric Properties of Jupiter Determined from Galilean Satellite Eclipse Light Curves.- Millisecond Polarized Pulses in Decametre-Wave Radiation from Jupiter and Sun.- The Atmosphere of Saturn.- Models of Saturn’s Rings which satisfy the Optical Observations.- A Study of the Outermost Ring of Saturn.- Theoretical Studies of an Atmosphere Around Saturn’s Rings.- The Saturnian ‘Gas-Doughnut’ Hypothesis.- Observational Constraints on Model Atmospheres for Uranus and Neptune.- Neptune: Observations of the H2 Quadrupole Lines in the (4–0) Band.- La rotation, la cartographie et la photométrie des satellites de Jupiter.- Optical Line Emission from Io.- Relation Between Light Variations of Solar System Satellites and Their Interaction with Interplanetary Medium.- IV / Future Explorations of the Solar System.- Spectroscopic Observations of Venus.- Photopolarimetry of Planets.- Rationale for NASAPlanetary Exploration Program.- Concluding Remarks.- Chairman’s Closing Remarks.- Index of Authors.

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