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Upper emission from

In all of these systems, the rate of generation at the gas-solid interface is so rapid that only a small fraction is canied away from the particle surface by convective heat uansfer. The major source of heat loss from the particles is radiation loss to tire suiTounding atmosphere, and the loss per particle may be estimated using unity for both the view factor and the emissivity as an upper limit from tlris source. The practical observation is that the solids in all of these methods of roasting reach temperatures of about 1200-1800 K. [Pg.283]

In Fig. 1.1, the parameter space for transient and stable cavitation bubbles is shown in R0 (ambient bubble radius) - pa (acoustic amplitude) plane [15]. The ambient bubble radius is defined as the bubble radius when an acoustic wave (ultrasound) is absent. The acoustic amplitude is defined as the pressure amplitude of an acoustic wave (ultrasound). Here, transient and stable cavitation bubbles are defined by their shape stability. This is the result of numerical simulations of bubble pulsations. Above the thickest line, bubbles are those of transient cavitation. Below the thickest line, bubbles are those of stable cavitation. Near the left upper side, there is a region for bubbles of high-energy stable cavitation designated by Stable (strong nf0) . In the brackets, the type of acoustic cavitation noise is indicated. The acoustic cavitation noise is defined as acoustic emissions from... [Pg.3]

Soil contributes to a greater extent to total carbon storage than do above-ground vegetation in most forests (Johnson and Curtis 2001). The total amount of soil organic carbon (SOC) in the upper meter of soil is about 1500 x 1015 g C (Eswaran et al. 1993 Batjes 1996), and the global atmospheric pool of CO2 is about 750 x 1015 g C (Harden et al. 1992). The CO2 emission from soil into atmosphere is about 68.0-76.5 1015 g C per year, and this is more than 10 times the CO2 released from fossil fuel combustion (Raich and Potter 1995). Variations in SOC pools and SOM turnover rates, therefore, exert substantial impacts on the carbon cycles of terrestrial ecosystems in terms of carbon sequestration in soil and CO2 emission from soil. [Pg.234]

Studies82 of the visible emission from shock-heated CS2 confirm this the temperature dependence of the emission shows that the upper state involved lies ap-... [Pg.58]

Exposure Levels in Environmental Media. Several studies are available documenting bromomethane concentrations in ambient air (Brodzinsky and Singh 1983 Harsch and Rasmussen 1977), but data for bromomethane in water are rare. Bromomethane has been analyzed for, but rarely detected, in foods (Daft 1987, 1988, 1989). Human exposure levels of bromomethane by inhalation of urban air have been calculated (Singh et al. 1981b). However, these levels are based on monitoring data more than 10 years old. Since urban air concentrations of bromomethane may have decreased due to reduced emissions from automobiles, exposure levels calculated from past data should be taken as an upper limit, and new levels calculated from current monitoring data would be useful. [Pg.79]

If an atomic transition is optically pumped by a beam of laser radiation having the appropriate frequency, the population in the upper state can be considerably enhanced along the path of the beam. This causes an intensification of the spontaneous emission from this state, which contains information about the conditions within the pumped region, since the exponential decay time for the intensified emission depends upon both the electron number density and the electron temperature. The latter can be obtained from the intensity ratio of the fluorescence excited from two different lower levels, if local thermal equilibrium is assumed. This method has been dis-... [Pg.54]

Emission from the upper electronic excited states of polyatomic molecules, in violation of Kasha s rule which allows emission only from the lowest excited states Q), have been observed in a reasonable variety of molecules (2 11). With notable exceptions of azulene and thioketone, however, such emission is usually very weak, because the rates of nonradiative decay processes greatly exceed the rates of radiative processes when excited states other than the lowest excited states are involved. [Pg.106]

Yellow flame color is achieved by atomic emission from sodium. The emission intensity at 589 nanometers increases as the reaction temperature is raised there is no molecular emitting species here to decompose. Ionization of sodium atoms to sodium ions will occur at very high temperatures, however, so even here there is an upper limit of temperature that must be avoided for maximum color quality. The emission spectrum of a yellow flare is shown in Figure 7.2. [Pg.197]

Flatpy, F., and 0. Hov, Three-Dimensional Model Studies of the Effect of NO, Emissions from Aircraft on Ozone in the Upper Troposphere over Europe and the North Atlantic, J. Geophys. Res., 101, 1401-1422(1996). [Pg.713]

Fig. 6. The emission from Ia(U3not(+)— -I2(ArlL/) + hr following the flash photolysis of CF3I as a function of wavelength and time, per = 2.0mmHg, = 80mmHg, E — 1767 J. Upper trace, I2(fi— X) emission lower trace, baseline. Wavelength scale 290 A per major division. Delay times (1) 2.0 msec, (2) 3.25 msec, (3) 4.5 msec. Fig. 6. The emission from Ia(U3not(+)— -I2(ArlL/) + hr following the flash photolysis of CF3I as a function of wavelength and time, per = 2.0mmHg, = 80mmHg, E — 1767 J. Upper trace, I2(fi— X) emission lower trace, baseline. Wavelength scale 290 A per major division. Delay times (1) 2.0 msec, (2) 3.25 msec, (3) 4.5 msec.
By using high intensity flash lamps and laser sources, photophysical and photochemical properties of the triplet states can be studied. These sources also help to study emission from upper excited state. [Pg.125]

The emission from electronically excited atomic and molecular oxygen is the cause of the night airglow. The atmospheric glow originates in the upper atmosphere where the pressure is so low that the radiative decay can compete favourably with the collisional deactivations. [Pg.224]

Estimated cost and C02 emissions for building 1.3-GW (gigawatt) power plants in 2000 and operating them tor 20 years. [Data from s. Pacca and A. Horvath, Greenhouse Gas Emissions from Building and Operating Electric Power Plants in the Upper Colorado River Basin, Environ. Sc/. Technol. 2002f 36,3194.]... [Pg.415]

In Situ Measurements Balloons. Balloons currently provide the only in situ platform that allows access to the upper part of the stratosphere (above 20 km). The engineering requirements are similar to those for aircraft except for a more relaxed time response. Regional coverage from balloons is difficult, particularly because the launching facilities for the large stratospheric balloons are very limited and generally localized in the midlatitudes. However, vertical profiles without horizontal distortion are the natural data collection mode. Measurement contamination due to emissions from the balloon is a potential problem. [Pg.265]

The situation at wavelengths below 2000 A has improved recently. The upper electronic state of benzene excited by absorption of the 1849-A line of mercury would be the 1 lu state.47 No light emission from this state has been reported and no evidence exists relative to crossover from this state to any of the various triplet states of lower energy. [Pg.347]

NOx emissions from subsonic aircraft flying in the troposphere and the lowermost stratosphere lead to a significant increase in ozone in the upper troposphere. Emissions of NOx and H20 from supersonic aircraft cruising in the stratosphere are calculated to decrease the column abundance of O3. The effects of aircraft emissions are found to be strongly dependent on flight altitudes and on assumed emission indices for NOx. [Pg.91]

In the study of chemiluminescence in elementary transfer reactions the behavior of the new-bond molecule has been emphasized over the past decade. This is understandable. The initial successful experiments showed new-bond excitation. Also, the work was conditioned by the observation of a highly non-thermal emission from OH in the upper atmosphere59 and the demonstration60 that a likely cause was the reaction H+03 -+ OH +Oj. Indeed, early work aimed at a test of the possibility that the principal excitation channel was via the highest accessible level. This hypothesis has not been proven. The available facts contradict it. Many levels of the new-bond molecule are populated by reaction. Ample evidence for this is provided by the reactions listed in Table 1. [Pg.132]


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Emissions from

Upper atmosphere, emission from

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