Flux density

For the field calculation it more convenient to use a tx(B) curve than the normal ix(H) curve because the calculated vector potential A is derived from the flux density B. This ii(B) curve however can be calculated easily from the measured values. [Pg.314]

The equation describes the manner in which the nuclear magnetization, M, at position r and time t processes about the magnetic flux density, B, in which it is found. The constant y is the magnetogyric ratio of the nuclides under study. The precessional frequency, co, is given by the Lannor equation. [Pg.1520]

Figure Bl.23.2. (a) Shadow cone of a stationary Pt atom in a 4 keV Ne ion beam, appearing with the overlapping of ion trajectories as a fiinction of the impact parameter. The initial position of the target atom that recoils in the collision is indicated by a solid circle, (b) Plot of the nonnalized ion flux distribution density across the shadow cone in (a). The flux density changes from 0 inside the shadow cone, to much greater than l in the focusing region, converging to 1 away from the shadow cone edge, (c) Blocking cones...

The electric discharge processes can supply the necessary energy very rapidly and convert more of the hydrocarbons to acetylene than in regenerative or partial combustion processes. The electric arc provides energy at a very high flux density so that the reaction time can be kept to a minimum (see... [Pg.384]

Technical Magnetic Behavior. When a magnetic-field strength H is appHed to a ferromagnetic or ferrimagnetic material, the latter develops a flux density or iaduction as a result of orientation of the magnetic domains. The relation between B and H is... [Pg.367]

B flux density, magnetic field, magnetic iaduction... [Pg.437]

P = total pressure atm. q = heat-flux density, energy per time-area. [Pg.570]

W = total leaving-flux density (also radiosity). [Pg.570]

The emissive power of a surface is the flux density (energy per time-surface area) due to emission from it throughout a hemisphere. If the intensity 7 of emission from a surface is independent of the angle of emission, Eq. (5-iii) may be integrated to showthat the surface emissive power is TC7, though the emission is throughout 2% sr. [Pg.570]

Variously called, in the literature, emittance, total hemispherical intensity, or radiant flux density. [Pg.570]

What is the sink-side efficiency T)i, the gas exit temperature Te, and the mean flux density through the tube surface ... [Pg.587]

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