RESEARCH REPORT OF ELEMENTAL ABUNDANCES OF THE LUNAR CRUST ACCORDING TO RECENT HYPOTHESES
Elemental abundances of the lunar crust
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Elemental abundances of the lunar crust
Possible elemental abundance of lunar crust - impact and volcanic origin
Origin of the lunar walled plain, ptolemaeus
Photographic measurement of craters in lunar walled plain ptolemaeus
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
Origin of the lunar walled plain ptolemaeus deduced from tectonic relations between diverse features in ptolemaeus and the grid systems in its vicinity
Possible origin of the lunar walled plain ptolemaeus
Lunar magnetic storm observations for separating solar event and earth environment effects in geomagnetic storms
Martian blue haze properties correlated with interplanetary dust, meteor showers and solar flares
Mechanisms causing increased brightness of lunar surface - solar flare proton and electron irradiation
Blue clearings of Mars atmosphere as function of number of meteor showers intersecting Mars orbit at intervals of heliocentric longitude
Lunar surface luminance transient enhancement noting photoabsorbing color center formation, increased reflectivity and photoluminescence, photoionization and photoemission
Correlation between mechanisms relating atmospheric heating and geomagnetic disturbances, examining temperature coefficient
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
Venus atmosphere carbon dioxide content origin from interior degassing during molten phase, using atmospheric model
Several techniques were employed to apply or otherwise form porous layers of various materials on the surface of hot-pressed silicon carbide ceramic. From mechanical properties measurements and studies, it was concluded that although porous layers could be applied to the silicon carbide ceramic, sufficient damage was done to the silicon carbide surface by the processing required so as to drastically reduce its mechanical strength. It was further concluded that there was little promise of success in forming an effective energy absorbing layer on the surface of already densified silicon carbide ceramic that would have the mechanical strength of the untreated or unsurfaced material. Using a process for the pressureless sintering of silicon carbide powders it was discovered that porous layers of silicon carbide could be formed on a dense, strong silicon carbide substrate in a single consolidation process.
Impact energy absorbing layers (EALs) comprised of partially densified silicon carbide were formed in situ on fully sinterable silicon carbide substrates. After final sintering, duplex silicon carbide structures resulted which were comprised of a fully sintered, high density silicon carbide substrate or core, overlayed with an EAL of partially sintered silicon carbide integrally bonded to its core member. Thermal cycling tests proved such structures to be moderately resistant to oxidation and highly resistant to thermal shock stresses. The strength of the developed structures in some cases exceeded but essentially it remained the same as the fully sintered silicon carbide without the EAL. Ballistic impact tests indicated that substantial improvements in the toughness of sintered silicon carbide were achieved by the use of the partially densified silicon carbide EALs.