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Thermalization track

Radiation chemical processes near the end of its thermalization track determine the environment in which the muon is found on an experimental time scale corresponding to its lifetime, = 2.2 ps. In experiments in transverse fields we distinguish between different components according to their signal amphtudes which are converted to fiactional muon polarizations Pi, with EPj = 1.0, if the fiill initial polarization in the beam is accounted for. [Pg.85]

Hydrocarbon-water contact movement in the reservoir may be determined from the open hole logs of new wells drilled after the beginning of production, or from a thermal decay time (TDT) log run in an existing cased production well. The TDT is able to differentiate between hydrocarbons and saline water by measuring the thermal decay time of neutrons pulsed into the formation from a source in the tool. By running the TDT tool in the same well at intervals of say one or two years (time lapse TDTs), the rate of movement of the hydrocarbon-water contact can be tracked. This is useful in determining the displacement in the reservoir, as well as the encroachment of an aquifer. [Pg.336]

The classical experiment tracks the off-gas composition as a function of temperature at fixed residence time and oxidant level. Treating feed disappearance as first order, the pre-exponential factor and activation energy, E, in the Arrhenius expression (eq. 35) can be obtained. These studies tend to confirm large activation energies typical of the bond mpture mechanism assumed earlier. However, an accelerating effect of the oxidant is also evident in some results, so that the thermal mpture mechanism probably overestimates the time requirement by as much as several orders of magnitude (39). Measurements at several levels of oxidant concentration are useful for determining how important it is to maintain spatial uniformity of oxidant concentration in the incinerator. [Pg.57]

Solar-thermal technology uses tracking mirrors to concentrate sunlight onto a receiver. In turn, the receiver absorbs solar energy as heat, warming a fluid that then drives a turbine generator. Most solar-thermal plants requite cooling water. [Pg.105]

Fig. 3. The 10-MW Solar One plant, which advanced solar thermal power through the use of tracking mirrors to concentrate sunlight onto a central... Fig. 3. The 10-MW Solar One plant, which advanced solar thermal power through the use of tracking mirrors to concentrate sunlight onto a central...
Hollomon s ethos, combined with his ferocious energy and determination, and his sustained determination to recruit only the best researchers to join his group, over the next 15 years led to a sequence of remarkable innovations related to materials, including man-made diamond, high-quality thermal insulation, a vacuum circuit-breaker, products based on etched particle tracks in irradiated solids, polycarbonate plastic and, particularly, the Lucalox alumina envelope for a metal-vapour lamp. (Of course many managers besides Hollomon were involved.) A brilliant, detailed account of these innovations and the arrangements that made them possible was later written by Guy Suits and his successor as director, Arthur Bueche (Suits and Bueche 1967). Some of these specific episodes will feature later in this book, but it helps to reinforce the points made here about Hollomon s coneeption of broad research on materials if I point out that the invention of translucent alumina tubes for lamps was... [Pg.9]

Fig. 46 Evaluation of the suitability of a hot plate for TLC by determination of the lemperature distribution. A) results of 25 thermal elements at temperature settings of 80 C, 100 C and 120 C, B) pattern of measuring points in five tracks (I—V) each with five measuring points... Fig. 46 Evaluation of the suitability of a hot plate for TLC by determination of the lemperature distribution. A) results of 25 thermal elements at temperature settings of 80 C, 100 C and 120 C, B) pattern of measuring points in five tracks (I—V) each with five measuring points...
For abrasion this is, however, a much more dominating process than for cut growth. The main reason is that the energy consumption in the abrasion process raises the temperature in the interface between rubber and track and thereby modifies this process. The temperature in the contact patch is a function of the power consumption and depends, therefore, also on the sliding speed. The temperature not only influences the oxidation and cut growth process, but also causes thermal degradation. [Pg.759]

Cool on-column Capillary Ramped temperature Track oven Low concentration or thermally labile Minimal sample discrimination and decomposition... [Pg.469]

It has been reported for many years that condensation nuclei can be produced by ionizing radiation. Recent studies have improved the measurement of the activity size distribution of these ultrafine particles produced by radon and its daughters (Reineking, et al., 1985 Knutson, et al., 1985). It seems that the Po-218 ion is formed by the radon decay, is neutralized within a few tens of milliseconds, and then attached to an ultrafine particle formed by the radiolysis generated by the polonium ion recoil. Although there will be radiolysis along the alpha track, those reactions will be very far away (several centimeters) from the polonium nucleus when it reaches thermal velocity. The recoil path radiolysis therefore seems to be the more likely source of the ultrafine particles near enough to the polonium atom to rapidly incorporate it. [Pg.368]

The foregoing analysis was for gas-phase water radiolysis. Similar estimates may be made for the condensed phases and for other media when the relevant yields and energetics become progressively available. On the whole, these species will gradually thermalize and become available for track reactions. Such reactions are greatly influenced by track structure, which is taken up in the following section. [Pg.50]

In liquefied rare gases (LRG) the ejected electron has a long thermalization distance, because the subexcitation electrons can only be thermalized by elastic collisions, a very inefficient process predicated by the small mass ratio of the electron to that of the rare gas atom. Thus, even at a minimum of LET (for a -1-MeV electron), the thermalization distance exceeds the interionization distance on the track, determined by the LET and the W value, by an order of magnitude or more (Mozumder, 1995). Therefore, isolated spurs are never seen in LRG, and even at the minimum LET the track model is better described with a cylindrical symmetry. This matter is of great consequence to the theoretical understanding of free-ion yields in LRG (see Sect. 9.6). [Pg.66]

FIGURE 9.3 A low-LET track in a liquefied rare gas (LRG). Even at a minimum LET, the electron thermalization length ( 103 nm) greatly exceeds the inter-positive-ion separation of R2+ ( 102 nm). Thus, the geometry approximates cylindrical symmetry rather than a collection of isolated ionizations. Reproduced from Mozumder (1995a), with the permission of Elsevier . [Pg.311]

Fig. 5.19. Evolutionary track in the HR diagram of an AGB model of total mass 0.6 Mq, initial composition (Y, Z) = (0.25, 0.001 Z /20). Heavy dots marked 2 to 11 indicate the start of a series of thermal pulses (see Fig. 5.20), which lead to excursions along the steep diagonal lines. Numbers along the horizontal and descending track indicate times in years relative to the moment when an ionized planetary nebula appears and (in parentheses) the mass of the envelope in units of Mq. R = 0.0285 indicates a line of constant radius (R in solar units) corresponding to the white-dwarf sequence. Shaded areas represent earlier evolutionary stages for stars with initial masses 3,5 and 7 Mq and the steep broken line marks the high-temperature boundary of the instability strip in which stars pulsate in their fundamental mode. The y-axis gives log L/Lq. Adapted from Iben and Renzini (1983). Fig. 5.19. Evolutionary track in the HR diagram of an AGB model of total mass 0.6 Mq, initial composition (Y, Z) = (0.25, 0.001 Z /20). Heavy dots marked 2 to 11 indicate the start of a series of thermal pulses (see Fig. 5.20), which lead to excursions along the steep diagonal lines. Numbers along the horizontal and descending track indicate times in years relative to the moment when an ionized planetary nebula appears and (in parentheses) the mass of the envelope in units of Mq. R = 0.0285 indicates a line of constant radius (R in solar units) corresponding to the white-dwarf sequence. Shaded areas represent earlier evolutionary stages for stars with initial masses 3,5 and 7 Mq and the steep broken line marks the high-temperature boundary of the instability strip in which stars pulsate in their fundamental mode. The y-axis gives log L/Lq. Adapted from Iben and Renzini (1983).

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See also in sourсe #XX -- [ Pg.89 ]




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