The evolution of Venus' atmosphere.
Venus atmosphere carbon dioxide content origin from interior degassing during molten phase, using atmospheric model
Engineering topics
Publications and source records attributed to Palm, A..
Venus atmosphere carbon dioxide content origin from interior degassing during molten phase, using atmospheric model
Planetary atmospheres data in 1967 for Venus, Mercury, Mars, Jupiter, Earth, and Moon
Valence force constants for nitric acid evaluated from fundamental mode vibration spectra by matrix method
Correlation between mechanisms relating atmospheric heating and geomagnetic disturbances, examining temperature coefficient
Lunar surface luminance transient enhancement noting photoabsorbing color center formation, increased reflectivity and photoluminescence, photoionization and photoemission
Mechanisms causing increased brightness of lunar surface - solar flare proton and electron irradiation
Martian blue haze properties correlated with interplanetary dust, meteor showers and solar flares
Blue clearings of Mars atmosphere as function of number of meteor showers intersecting Mars orbit at intervals of heliocentric longitude
Lunar magnetic storm observations for separating solar event and earth environment effects in geomagnetic storms
Origin of the lunar walled plain ptolemaeus deduced from tectonic relations between diverse features in ptolemaeus and the grid systems in its vicinity
Measurements of the diameters of craters in the lunar walled plain ptolemaeus and in vicinal equal-area terrae /highland surfaces/ by currently available lunar photographs
Photographic measurement of craters in lunar walled plain ptolemaeus
Possible origin of the lunar walled plain ptolemaeus
Origin of the lunar walled plain, ptolemaeus
Possible elemental abundance of lunar crust - impact and volcanic origin
Elemental abundances of the lunar crust