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International Ultraviolet

Fig. 8.3. C/O ratio vs. O/H in Galactic and extragalactic H n regions, based on International Ultraviolet Explorer (IUE) and Hubble Space Telescope (HST) observations. After Garnett (2004). Fig. 8.3. C/O ratio vs. O/H in Galactic and extragalactic H n regions, based on International Ultraviolet Explorer (IUE) and Hubble Space Telescope (HST) observations. After Garnett (2004).
Walborn, N. R., Nichols-Bohlin, J., and Panek, R. J. 1985, International Ultraviolet Explorer Atlas of O-Type Spectra from 1200 to 1900 A, NASA RP-1155. [Pg.78]

Flow diagram of Ultrox system. (From USEPA, Ultrox International Ultraviolet Radiation/ Oxidation Technology—Applications Analysis Report, EPA/540/A5-89/012, September 1990.)... [Pg.550]

Effect of hydrogen peroxide on ozone treatment system at ozone production rates of 10.5 and 15.7 lb/day. The x-axis shows the hydrogen peroxide-to-ozone mass ratio. The treatment efficiency report is the sum of oxidation and air stripping. (From USEPA, Ultrox International Ultraviolet Radiation/Oxidation Technology—Applications Analysis Report, EPA/540/A5-89/ 012, September 1990.)... [Pg.576]

Ultraviolet technologies, applications, research International Ultraviolet Association (lUVA) http II WWW. iu va. 0 rg... [Pg.9]

Rice RG (2001) Practical Applications of UV in Combination with Ozone, Conference Proceedings of the First International Congress on Ultraviolet Technologies, International Ultraviolet Assoc. (lUVA), June 14-16, Washington, DC electronic release. [Pg.16]

Technologies, International Ultraviolet Assoc. (lUVA), June 14-16, Washington, DC, electronic release. [Pg.98]

Ackermann, 1971) and for two additional values 300 times the present value and for the wavelength-dependent ultraviolet flux emitted by early sun-like stars (T-Tauri) as observed with the International Ultraviolet Explorer (lUE) satellite (Canuto et al., 1982, and Canuto et al., 1983). The model extends from the surface to 53.5 km with 1 kilometer spatial resolution between the surface and 10 km, and 1.5 kilometers spatial resolution between 10 and 53.5 km. Further details about the model are given in Levine et al. (1981) and Levine et al. (1982). [Pg.84]

Nelson R. M., Lane A. L., Matson D. L., Veeder G. J., Buratti B. J., and Tedesco E. F. (1987) Spectral geometric Albedos of the Galilean satellites from 0.24 to 0.34 micrometers— observations with the international ultraviolet explorer. Icarus 72, 358-380. [Pg.653]

Internal combustion engine International Space Station International Ultraviolet Explorer Internet file transfer and tracking Internet and the World Wide Web Interstellar matter Interval... [Pg.16]

See other pages where International Ultraviolet is mentioned: [Pg.107]    [Pg.481]    [Pg.71]    [Pg.406]    [Pg.67]    [Pg.4]    [Pg.16]    [Pg.186]    [Pg.235]    [Pg.290]    [Pg.291]    [Pg.291]    [Pg.298]    [Pg.83]    [Pg.75]    [Pg.166]    [Pg.59]    [Pg.164]   


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International Ultraviolet Explorer

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