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Flux energy

The energy flux in a uniform anisotropic medium is stiU given by the Poynting vector [Pg.66]

Because in general , is not perpendicular to s, Si is not parallel to s. For a light beam, if the initial polarization is not an eigenmode, then the electric field can be decomposed into the two eigenmodes  [Pg.66]

Hence s-S =s- 2 2, indicating that the total energy flux in the propagation direc- [Pg.67]


Since the absorption spectrum is a ratio it is amenable to other interpretations. One such interpretation is that the absorption spectrum is the ratio of energy absorbed to energy incident. From this perspective, the quantity /)co(d/d0< li 0l f 0) is interpreted as the rate of energy absorption (per unit volume), since d E/d t = /)co(d AVd t) while tire quantity E dha is interpreted as the incident energy flux, which depends only on the field intensity and is independent of frequency. [Pg.245]

Sound energy flux p, p. chemical cell reaction ... [Pg.107]

Spectral radiant energy flux d(j)/dk Surface pressure 7T... [Pg.107]

The nonconvective energy flux across the boundary is composed of two terms a heat flux and a work term. The work term in turn is composed of two terms useful work deflvered outside the fluid, and work done by the fluid inside the control volume B on fluid outside the control volume B, the so-called flow work. The latter may be evaluated by imagining a differential surface moving with the fluid which at time 2ero coincides with a differential element of the surface, S. During the time dt the differential surface sweeps out a volume V cosdSdt and does work on the fluid outside at a rate of PV cos dS. The total flow work done on the fluid outside B by the fluid inside B is... [Pg.109]

Because the evaporation of the solvent is an endothermic process, heat must be suppHed to the system, either through conduction, convection, radiation, or a combination of these methods. The total energy flux into a unit area of coating, is the sum of the fluxes resulting from conduction, convection, and radiation (see Heat exchange technology, HEAT thansfer). [Pg.314]

The spectral distribution of energy flux from a black body is expressed by Planck s law ... [Pg.570]

Radiated energy flux Energy flux to a black body Flow rate... [Pg.717]

Pyrometers Planck s distribution law gives the radiated energy flux qb(X, T)dX in the wavelength range X to X -1- dX from a black surface ... [Pg.760]

Ratio Pyrometers The ratio pyrometer is also called the two-color pyrometer. Two different wavelengths are utilized for detecting the radiated signal. If one uses Wien s law for small values of XT, the detected signals from spectral radiant energy flux emitted at the wavelengths and 2 with emissivities and are... [Pg.761]

V is the material velocity. a is the stress tensor. g is the acceleration of gravity. e is the internal energy per unit mass. h is the energy flux. [Pg.326]

The sun radiates approximately as a blackbody, with an effective temperature of about 6000 K. The total solar flux is 3.9 x 10 W. Using Wien s law, it has been found that the frequency of maximum solar radiation intensity is 6.3 x 10 s (X = 0.48 /rm), which is in the visible part of the spectrum 99% of solar radiation occurs between the frequencies of 7.5 X 10 s (X = 4/um) and 2 x 10 s (X = 0.15/um) and about 50% in the visible region between 4.3 x 10 s (X = 0.7 /rm) and 7.5 X 10 s (X = 0.4 /Ltm). The intensity of this energy flux at the distance of the earth is about 1400 W m on an area normal to a beam of solar radiation. This value is called the solar constant. Due to the eccentricity of the earth s orbit as it revolves around the sun once a year, the earth is closer to the sun in January (perihelion) than in July (aphelion). This results in about a 7% difference in radiant flux at the outer limits of the atmosphere between these two times. [Pg.246]

IFIGURE IL36 Th room model characterizes the individua) energy flux paths as thermal resistances. which are connected to the individual surfaces and to the room air node. [Pg.1071]

Wind turbines produce power by converting the force of the wind into torque. The power produced is a function of the wind energy flux (power), which, in turn, is a function of the air density multiplied by the wind velocity raised to the third power. Changes of air density with time at a particular site are negligible compared to the fluctuations in wind velocity. Meteorologists usually report wind speed as an average. To get the potential wind power, the average... [Pg.92]

Fig. 17-1 The global climate system, (a) Energy fluxes, including incoming solar radiation, reflected radiation, emitted longwave radiation (from an effective altitude of ca. 6 km), and atmospheric and oceanic heat flux toward the polar regions, (b) The atmospheric circulation corresponding to part (a). Refer back to Fig. 7-4 and associated text for a discussion of the general circulation. Fig. 17-1 The global climate system, (a) Energy fluxes, including incoming solar radiation, reflected radiation, emitted longwave radiation (from an effective altitude of ca. 6 km), and atmospheric and oceanic heat flux toward the polar regions, (b) The atmospheric circulation corresponding to part (a). Refer back to Fig. 7-4 and associated text for a discussion of the general circulation.
TOWARDS THE HYDRODYNAMIC LIMIT STRUCTURE FACTORS AND SOUND DISPERSION. The collective motions of water molecules give rise to many hydrodynamical phenomena observable in the laboratories. They are most conveniently studied in terms of the spatial Fourier ( ) components of the density, particle currents, stress, and energy fluxes. The time correlation function of those Fourier components detail the decay of density, current, and fluctuation on the length scale of the Ijk. [Pg.246]

Figure 8.30. Theoretical energy flux for radiation from the sun as a black body at 5,800 K. The spectrum reaching the surface of the earth is modified through absorption in the infrared region by H2O and CO2 and in the... Figure 8.30. Theoretical energy flux for radiation from the sun as a black body at 5,800 K. The spectrum reaching the surface of the earth is modified through absorption in the infrared region by H2O and CO2 and in the...
Direct photochemical reactions in the stratosphere induced by far ultraviolet solar light are well known to be important for the chemistry of the atmosphere. However, only a small fraction of the solar energy flux is in this spectral region. [Pg.48]

The maximum kinetic energy flux of ions. (eTlmax (W m ), can be defined as... [Pg.118]

FIG. 45. (a) The ratio of the ion flux to the deposition flux. Rj. and (b) the ratio of the energy flux to the deposition flux. max. as a function of power delivered to the SiHa-Ar discharge at an excitation frequency of 50 MHz and a pressure of 0.4 mbar. (Compiled from E. A. G. Hamers. Ph.D. Thesis. Universiteit Utrecht. Utrecht, the Netherlands. 1998.)... [Pg.121]


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Convective flux internal energy

Energy continued flux functions

Energy flux density spectrum

Energy flux rate

Energy flux vector

Energy flux vector expression

Energy flux, collisional contribution

Energy flux, components

Energy flux, saturation

Energy flux, solar radiation

Energy spectrum scalar-flux

Expected Solar Neutrino Sources, Energies, and Fluxes

Ignition, energy flux

Maintenance energy flux

Mass-energy flux

Molecular flux thermal energy

Momentum and Energy Fluxes

Solar energy flux

Spatial and Temporal Characteristics of the Type I ELM Energy Fluxes to PFCs

Surface energy flux vector

Water evaporation energy flux

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