Planetary Atmospheres: A Continuing Bibliography |
From inside the book
Results 1-3 of 43
Page 13
... thermal emission . The main factor determining the " quiet " or " glow " atmospheric discharge on Venus would not be the electrical - storm phenomena characteristic for the earth , but may be the extremely slow rotation of the planet ...
... thermal emission . The main factor determining the " quiet " or " glow " atmospheric discharge on Venus would not be the electrical - storm phenomena characteristic for the earth , but may be the extremely slow rotation of the planet ...
Page 45
... thermal opacity was provided by the pressure - induced absorption of H2 and also by its enhancement resulting from mixing with He . The thermal opacity due to NH 3 was found to be negligible in all of the major planets except Jupiter ...
... thermal opacity was provided by the pressure - induced absorption of H2 and also by its enhancement resulting from mixing with He . The thermal opacity due to NH 3 was found to be negligible in all of the major planets except Jupiter ...
Page 34
... THERMAL PLASMA MODEL FOR DISTRIBUTION OF THERMAL PLASMA IN MAGNETOSPHERE OF JUPITER UNDER ASSUMPTION OF COROTATION WITH PLANET A67-33196 THERMAL PROPERTY TIDAL OSCILLATION THERMAL STRUCTURE OF UPPER MARS ATMOSPHERE NASA - TM - X - 57327 ...
... THERMAL PLASMA MODEL FOR DISTRIBUTION OF THERMAL PLASMA IN MAGNETOSPHERE OF JUPITER UNDER ASSUMPTION OF COROTATION WITH PLANET A67-33196 THERMAL PROPERTY TIDAL OSCILLATION THERMAL STRUCTURE OF UPPER MARS ATMOSPHERE NASA - TM - X - 57327 ...
Contents
STAR Abstracts | 1 |
IAA Abstracts | 29 |
Aerospace Medicine and Biology Abstracts | 57 |
1 other sections not shown
Other editions - View all
Common terms and phrases
absorption ABUNDANCE Aeronautics American analysis APPLICATION Astronautical Astrophysical ATMOSPHERE MODELS atmosphere of Venus Author bands BRIGHTNESS CALCULATION Calif CARBON DIOXIDE Center CFSTI CHARACTERISTICS CIRCULATION cloud compared COMPONENT COMPOSITION computed considered CONTENT Contract CSCL density DESIGN DETERMINATION developed discussed distribution dust EARTH EFFECT EMISSION ENTRY equations equilibrium estimates experiment field Flight FREQUENCY function given Grant heat indicate Institute International IONOSPHERE Journal JUPITER Laboratory layer limit lines MARINER MARS ATMOSPHERE MARTIAN ATMOSPHERE Mass mean MEASUREMENTS method MICROWAVE mission NASA NOTING OBSERVATIONS obtained OCCULTATION optical ORBITER PARAMETERS particles PHYSICS planet PLANETARY ATMOSPHERES POLARIZATION presented PROBE problem PROGRAM PROPERTIES radiation radiative RADIO range REFLECTION refs region Report Research rotation SCATTERING Sciences SIMULATED SOLAR Space SPECTRAL SPECTROSCOPIC spectrum STRUCTURE surface pressure Technology temperature THERMODYNAMIC tion University UPPER ATMOSPHERE values variations VEHICLE VENUS ATMOSPHERE Washington WATER VAPOR York