Big Chemical Encyclopedia

Chemical substances, components, reactions, process design ...

Articles Figures Tables About

Radiational cooling

An inversion caused by mixing in a surface layer was just discussed above. Inversions at the surface are caused frequently at night by radiational cooling of the ground, which in turn cools the air near it. [Pg.256]

Just as heating in the daytime occurs more quickly over land than over water, at night radiational cooling occurs more quickly over land. The pressure pattern tends to be the reverse of that in the daytime. The warmer air tends to rise over the water, which is replaced by the land breeze from land to water, with the reverse flow (water to land) completing the circular flow at altitudes somewhat aloft. Frequently at night, the temperature differences between between land and water are smaller than those during the daytime, and therefore the land breeze has a lower speed. [Pg.263]

At night when radiational cooling occurs on slopes, the cool dense air near the surface descends along the slope (Fig. 17-19). This is the downslope wind. To compensate for this descending air, air farther from the slope that is cooled very little is warmer relative to the descending air and rises, frequently resulting in a closed circular path. Where the downslope winds... [Pg.263]

Fig. 17-19. Downslope wind (night) due to more rapid radiational cooling on the valley s slope than in its center. Fig. 17-19. Downslope wind (night) due to more rapid radiational cooling on the valley s slope than in its center.
Electrical isolation Heat radiation Cooling coils Recent incidents Vacuum relief valves Accidents at sea Fires Problem sources Emulsion breaking Chimney effects Interlock failure Choosing materials. [Pg.410]

Fiber reinforcement of polymers allows us to use them in engineering applications that were previously off limits, We use fiber reinforced injection moldings in many under-the-hood automotive applications, such as rocker box covers and front end modules, which support the radiator, cooling fan, and hood latch, that are subjected to a wide range of temperatures. [Pg.248]

Fermentation temperatures are not critical in producing shermat but, of course, temperatures should be below about 30° C to produce a sound wine. Fermentations are conducted in large tanks, usually over 40,000 gallons. Since very little heat is lost by radiation, cooling is necessary for processing shermats that are fermented to dryness. [Pg.145]

Ne (-) (o) (+) candidate for radiation cooling with recycling excitation rates needed... [Pg.156]

For the hydrogenation of ethylene, the activities of nickel and platinum were observed after various surface treatments of argon-ion bombardment, radiation cooling, and annealing (38). Activities for the ion bombarded surfaces were as great as 10 times those for annealed surfaces while those for the radiation-cooled surfaces were 2-3 times the annealed values, thus indicating the role of lattice defects in this type of reaction. [Pg.59]

Urea and potassium bicarbonate Potassium chloride Potassium bicarbonate Sodium bicarbonate Chemically inhibits combustion chain reaction Blocks radiation Cooling Flammable and combustible liquids Electrical fires Ordinary commodities Metals... [Pg.123]

The ground (z = 0) temperature is governed by solar heating during the day and radiational cooling during the night. Therefore 0(0, t) may be expressed as... [Pg.758]

It was still too hot for the electrons to join the hydrogen and helium ions to form neutral atoms. This occurred not until about 500 000 years later, wh tenq>erature had dropped to a few 1000 K. The disappearance of free electrons broke the thermal contact between radiation and matter, and radiation continued then to expand freely. An outside spectator would have observed this as a hugh flash and a rapidly expanding fireball. In the adiabatic expansion the radiation cooled further to the cosmic background radiation level of 2.7 K measured today. [Pg.449]

Radiation Power Rate. For sources consisting of a known weight of a single radioisotope whose decay properties are known, the power in Mev/g-sec can be computed from Eq. (10-14) or (10-16). Conversion to watts is then made on the basis that 1 Mev/sec = 1.6 X 10 watt. The addition of other radioisotopes to the volume source requires a summation of the power value calculated for each isotope as described. The power liberation from a complex mixture of radioisotopes such as found in the fission products of U fuel is time-consuming to calculate. Figure 10-7 avoids the necessity of this by giving the and y power, curies and composition of the radioactive isotopes, all as a function of elapsed time after the fuel is pulled from the reactor. This elapsed time is known as the radiation cooling period. [Pg.445]

The TBS utilises both a passive radiator cooling system and a semi-active system comprising heaters and thermal sensors that are controlled and managed by the Thermal Control Unit (TCU). MLI is used to thermally decouple the experiment from deep space and solar effects. Thermal screens consisting of Kapton foil (X-Ray transparent) are interposed in the telescopes field of... [Pg.165]

Radiational cooling The phenomenon of enhanced loss of heat from Earth on a clear, cloudless night due to the absence of significant water vapor in the atmosphere in the form of clouds... [Pg.133]

What is radiational cooling On what type of night might this phenomenon be least noticeable ... [Pg.137]


See other pages where Radiational cooling is mentioned: [Pg.263]    [Pg.563]    [Pg.616]    [Pg.777]    [Pg.6]    [Pg.18]    [Pg.315]    [Pg.176]    [Pg.398]    [Pg.10]    [Pg.141]    [Pg.152]    [Pg.156]    [Pg.156]    [Pg.156]    [Pg.294]    [Pg.224]    [Pg.136]    [Pg.644]    [Pg.59]    [Pg.269]    [Pg.31]    [Pg.188]    [Pg.493]    [Pg.774]    [Pg.113]    [Pg.133]    [Pg.140]   
See also in sourсe #XX -- [ Pg.133 ]




SEARCH



Cooling by radiation

Radiation and convection cooling of the substrate

Radiation cooling

Terrestrial radiation cooling

© 2024 chempedia.info