4 Chemical composition, 5 Flexibility and apertures, 6 Other information

Author(s):  
W. H. Baur ◽  
R. X. Fischer

Author(s):  
K. E. Pitjeva ◽  
E. I. Baranovskaya

The article provides information about the chemical composition of groundwater and the data of chemical analysis, the water extracts from rocks, and other information, that characterize water and rocks in the depth range of water-saturated riphean deposits. The article discusses the natural background conditions of distribution of hydrocarbon sorbing gases in atmohydrolithosphere and the conditions of oil and gas accumulations, under the influence of which sorbed hydrocarbon gases acquire specific geochemical features.



2014 ◽  
Vol 608 ◽  
pp. 37-40
Author(s):  
Toyohiko Sugiyama

In the research of ceramic glazes, the process of preparing the glaze test pieces and improving the recipe is repeated. Our institute, AIST Japan, has more than 300,000 glaze test pieces from over 80 years of ceramic studies. These pieces are the physical evidence of the processes and the results of glaze test experiments. As such, they provide valuable information for glaze and ceramic research. The Ceramic Color Database has been constructed to make this fundamentally important information widely accessible in support of R&D in the ceramics industry. The database includes: glaze name, firing temperature, firing atmosphere, coloring, chemical composition, recipe, physical state, and other information, as well as images of the glaze pieces. The database has been used in recent ceramics research, and its effectiveness has been verified. It was also recognized that the vast amount of data provided by the database is useful in the material development and basic research of fields other than ceramics. The database has been improved based on such usage status. In this paper, the structure and usage of the database are described and the future development of the database is discussed.



1983 ◽  
Vol 6 ◽  
pp. 119-127
Author(s):  
Francois Spite

The abundance of the elements in the halo are mostly known from analysis of stellar atmospheres. Data from evolved stars and planetary nebulae have to be used with some caution. I will therefore rely primarily on unevolved cool dwarfs, using other information only as a complement.I will designate these unevolved cool dwarfs indifferently by the words halo dwarfs or Population II dwarfs; such stars were formerly often called subdwarfs for historical reasons. Remaining in the field of vocabulary, I will call underdeficient an element which is deficient, but by a factor smaller than the general deficiency factor for the other elements. Finally, let us recall the classical notation:



1962 ◽  
Vol 14 ◽  
pp. 149-155 ◽  
Author(s):  
E. L. Ruskol

The difference between average densities of the Moon and Earth was interpreted in the preceding report by Professor H. Urey as indicating a difference in their chemical composition. Therefore, Urey assumes the Moon's formation to have taken place far away from the Earth, under conditions differing substantially from the conditions of Earth's formation. In such a case, the Earth should have captured the Moon. As is admitted by Professor Urey himself, such a capture is a very improbable event. In addition, an assumption that the “lunar” dimensions were representative of protoplanetary bodies in the entire solar system encounters great difficulties.



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