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Stars power

Finally, Network, network, network. Sound familiar We talked about enlisting males and people with star power as allies in what you need to accomplish. [Pg.129]

As research on fusion weapons was going on, attempts were also being made to develop peaceful uses for nuclear fusion. The concept of a star power plant just outside the city was never out of sight for a number of nuclear scientists. [Pg.588]

The rms noise is measured in a noise bandwidth, The D is called D star lambda when the spectral band is limited to a given interval, and D blackbody when the total blackbody incident power density is used in the calculation. [Pg.422]

Voltage polarization depends upon the location of the relay and the location of the fault. It is possible that the residual voltage, at a particular location in the system, is not sufficient to actuate the voltage coil of the directional G/F relay. In such an event, current polarization is used to supplement voltage polarization. Current polarization is possible, provided that a star point is created on the system, even through a A/t> power transformer, if such a transformer is available in the same circuit. Figure 21.20. Else a grounding transformer may be provided as... [Pg.691]

It is common practice to leave the star-connected capacitor banks ungrounded when used in the system or use delta-connected banks to prevent the flow of third harmonic currents into the power system through the grounded neutral. [Pg.734]

Industrial Power Engineering and Applications Handbook Conversion from delta to star... [Pg.758]

Power Plants—Scientist Labels New Ozone Threats , Newark Star Ledger, Newark, NY, 17 (Nov 15, 1975)... [Pg.316]

The scarcity of data and their invaluable content require that they be recorded in the most careful manner. The human eye is an incredibly powerful and versatile instrument, with an amazing dynamic range. But almost the entire universe is beyond its reach. Modem telescopes have a sensitivity 9 to 10 order of magnitude higher, yet they are barely able to provide a glimpse at the youngest galaxies, least to say stars. [Pg.21]

Sodium Guide Star Brightness. From the properties of the Na atom and the Na layer (Table 1), we can estimate the power needed for the AO system. Assuming isotropic emission and no saturation, the photon flux F of the LGS observed with the WFS is given by ... [Pg.220]


See other pages where Stars power is mentioned: [Pg.414]    [Pg.7]    [Pg.657]    [Pg.174]    [Pg.178]    [Pg.184]    [Pg.449]    [Pg.414]    [Pg.7]    [Pg.657]    [Pg.174]    [Pg.178]    [Pg.184]    [Pg.449]    [Pg.1242]    [Pg.3]    [Pg.338]    [Pg.150]    [Pg.373]    [Pg.75]    [Pg.240]    [Pg.291]    [Pg.668]    [Pg.746]    [Pg.760]    [Pg.819]    [Pg.482]    [Pg.483]    [Pg.276]    [Pg.425]    [Pg.80]    [Pg.154]    [Pg.589]    [Pg.760]    [Pg.802]    [Pg.849]    [Pg.871]    [Pg.901]    [Pg.901]    [Pg.901]    [Pg.902]    [Pg.749]    [Pg.31]    [Pg.206]    [Pg.212]    [Pg.226]    [Pg.243]   
See also in sourсe #XX -- [ Pg.60 , Pg.89 ]




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