Big Chemical Encyclopedia

Chemical substances, components, reactions, process design ...

Articles Figures Tables About

Gaseous sources

Figure 9.20 A gaseous source-sink mapping diagram for (he ammonium nitrate example... Figure 9.20 A gaseous source-sink mapping diagram for (he ammonium nitrate example...
Ho and L. A. Kolodziejski, Gaseous Source UHV Epitaxy Technologies for Wide Bandgap II-VI Semiconductors... [Pg.302]

S. Fujita and S. Eujita, Growth and Characterization of ZnSe-based II-VI Semiconductors by MOVPE E. Ho and L. A. Kolodziejski, Gaseous Source UHV Epitaxy Technologies for Wide Bandgap II-VI Semiconductors... [Pg.190]

Robertson, J.B., 1969. Diffusion from a gaseous source in a porous medium. A field and theoretical comparison. US Geol. Survey, Prof Pap., 650-D 265-273. [Pg.500]

M. Komori, T. Maid, T. Kim, G. Hou, Y. Sakaguchi, K. Sakuta, and T. Kobayashi, Homoepitaxial growth of diamond thin films by electron cyclotron-resonance microwave plasma chemical-vapor-deposition apparatus with CO/H gaseous source, Appl. Phys. Lett., 62(6) 582-584 (1993)... [Pg.168]

Table 5-2. Physical and harzard properties of common gaseous sources for CVD of dielectric materials. Table 5-2. Physical and harzard properties of common gaseous sources for CVD of dielectric materials.
It is sometimes desirable to prepare gaseous compounds of lead for mass spectrographic analysis or for measurement of decay characteristics. In particular the study of long lived (5 X 10, yr) lead-205 which decays by electron capture unaccompanied by gamma ray emission or of other electron-capture Isotopes Is facilitated by the use of a gaseous source which can be Introduced directly into the counting chamber for increased detection efficiency. [Pg.108]

The Pioneer Venus mission (1978) explored the atmosphere of Venus. One of the payloads was a GC system equipped with two gas columns and a TCD detector. Tlie system was used to analyze samples of the atmosphere during the probe s descent to determine the composition of Venus lower atmosphere. From these measurements, deductions were made of the gaseous sources of infrared opacity, the degree of differentiation of Venus interior, the degree of similarity between the solid bodies of Earth and Venus, and the evolution of Venus atmosphere to determine the composition atmospheric composition measurements [50]. [Pg.397]

See other pages where Gaseous sources is mentioned: [Pg.163]    [Pg.467]    [Pg.491]    [Pg.471]    [Pg.1135]    [Pg.520]    [Pg.456]    [Pg.422]    [Pg.429]    [Pg.196]    [Pg.3]    [Pg.1371]    [Pg.351]    [Pg.396]    [Pg.109]    [Pg.116]    [Pg.407]    [Pg.267]    [Pg.104]    [Pg.55]    [Pg.1370]    [Pg.4]    [Pg.304]    [Pg.468]    [Pg.155]    [Pg.468]    [Pg.326]    [Pg.123]    [Pg.118]    [Pg.119]    [Pg.64]    [Pg.64]    [Pg.71]    [Pg.89]    [Pg.219]    [Pg.696]   
See also in sourсe #XX -- [ Pg.270 ]



SEARCH



© 2024 chempedia.info