THE STUDY OF PLANETARY ATMOSPHERES BY STELLAR OCCULTATION
Study of planetary atmospheres by stellar occultation
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Study of planetary atmospheres by stellar occultation
Atmospheric sounding by satellite measurements of stellar refraction
Stellar spectrum lines - formation and intensity
Test for the verification of the dynamo theory of earth and stellar magnetism
Stellar spectra and ultraviolet auroral observations by aerobee rockets in the 1,300-1,800 angstrom region
Ultraviolet aurora with north-south asymmetry and stellar spectra taken from aerobee rocket flight
Distribution of meteors according to stellar magnitude
Comments on huang theory of probability of planet position near a star and on the location of stellar life zones
Termination of proton-proton chain in stellar interiors, noting influence of deuterium and helium 3 burning reactions
Relationship between chemical composition and photometric metal index in stellar atmospheres
Ultraviolet rocket spectrometer for measuring stellar spectra
Nongray stellar atmosphere boundary temperature in terms of absorption coefficients
Satellite measurement of atmospheric structure by stellar refraction, starlight transmission through atmosphere, and background sky brightness
Line blanketing attenuation of stellar UV RADIATION from rocket observation, noting B-star atmosphere
Nuclear reactions replacing gravitational contraction as major source of stellar luminosity for model stars and approach to main sequence
Redshift of quasi-stellar radio source 3C 286 determined by prime-focus photoelectric spectrum scanner, considering emitting elements for various lines