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Temperature in the atmosphere

Total Mass, Moles, and Molecules of the Atmosphere The total mass of the atmosphere is [Pg.11]

An estimate for the total number of moles of air in the atmosphere is total mass/Mair Total moles 1.62 x 1020 mol [Pg.11]

An accurate estimate of the total mass of the atmosphere can be obtained by considering the global mean surface pressure (985.50hPa) and the water vapor content of the atmosphere (Trenberth and Smith 2005). The total mean mass of the atmosphere is [Pg.11]

The mean mass of water vapor in the atmosphere is estimated as 1.27 x 1016 kg, and the dry air mass of the atmosphere is [Pg.11]

Pole (90° latitude) are colder than those over the South Pole (—90° latitude) the reverse is true in July. [Pg.12]


The silicon detectors were made of n-typed single crystal of 1 mm thick. They have a MOS structure of gold, tungsten oxide, n-typed silicon and aluminum back contact. Since these layers can be deposited on the silicon wafer by evaporation techniques, the fabrication process is so simple as to be applicable to fabrication of the detectors for a special use. No surface treatment for passivation is given to them so that their performance is affected by ambient gases. For example, some good detectors show a leakage current of half micro-ampere at room temperature in the atmosphere, but a few micro-ampere in vacuum. So, in order to stabilize their performance, the silicon detectors were operated at the dry ice temterature. [Pg.491]

A recent laboratory comparison of the shape of the water of hydration bands with the spectra obtained by the Galileo spacecraft indicates that the hydrated material mentioned above might in fact be frozen, hydrated H2S04. This material would be produced by the charged particle irradiation of sulfate salts, sulfur or SO2 in an ice matrix. Therefore, a sulfur chemical cycle is maintained by the incident radiation, a cycle similar to that occurring at higher temperatures in the atmospheres of the Earth and Venus. On Europa, this involves oxidants such as SO ", H202 and 02 which have potential importance for the proposed prebiotic chemistry. [Pg.393]

Rayleigh model. The three sets of curves are for different initial sea surface temperatures (T ). The approach of Merhvat and Jouzel (1979) is used for the liquid phase, and that of Jouzel and Merlivat (1984) is used for snow formation. The sohd lines correspond to East Antarctic data plotted with respect to either Ts (surface temperature) or 7) (temperature in the atmosphere at the inversion level). [Pg.2135]

Nonetheless, some approximate values for the nature and composition of the lunar atmosphere have been obtained. Temperatures in the atmosphere vary widely, from a low of about 100 K (—173°C) during the lunar night to a high of about 400 K (127°C) during the lunar day. Surface pressure at night on the Moon is about 3 x 10 15 bar, or about one quadrillionth that on Earth. There are about 2 x 10s particles per cubic centimeter at the Moon s surface. [Pg.218]

The temperature in the atmosphere varies by less than a factor of 2, while the pressure changes by six orders of magnitude (see Table A.8). If the temperature can be taken to be... [Pg.9]

Water is abundant on our planet, distinguishing Earth from all other planets in the solar system. More than 97% of Earth s water is in the oceans, with 2.1% in the polar ice caps and 0.6% in aquifers. The atmosphere contains only about one part in a hundred thousand (0.001%) of Earth s available water. However, the transport and phase distribution of this relatively small amount of water (estimated total liquid equivalent volume of 13,000 km3) are some of the most important features of Earth s climate. The existence of varying pressures and temperatures in the atmosphere and at the Earth s surface causes water to constantly transfer among its gaseous, liquid, and solid states. Clouds, fogs, rain, dew, and wet aerosol particles represent different forms of that water. Aqueous atmospheric particles play a major role in atmospheric chemistry, atmospheric radiation, and atmospheric dynamics. [Pg.284]

Although p0 and Tq in (16.39) refer to the constant surface values, equations of precisely the same form can be derived in which p0 and 7o are replaced by pe and Te, the reference profiles. The equations written in this form will be useful later when we consider the dynamics of potential temperature in the atmosphere. [Pg.736]

Temperature in the atmosphere varies with location on the surface and elevation. Figure 1.4 shows the mean temperature over the period 1980 to 1989 between 1000 mbar and 50 mbar averaged around a latitude band. Highest values occur in the tropics at the 1000 mbar level... [Pg.16]

One can use a roll mill to prepare the plastic/rubber blends, using heated rolls, in the laboratory. However, for production this may be very cumbersome and, since the polymers are melt-mixed at high temperature in the atmosphere, handling of the molten polymer and degradation by heat could be an issue. Quality consistency could be another issue with this process. [Pg.114]

An additional feature that is closely related to syngas generation is the development of carbon capture and sequestration (CCS) that is initiated by the increased CO2 concentration in the atmosphere, and the increased understanding about increased CO2 levels that are contributing to the increased average temperature in the atmosphere. [Pg.2043]

What is the role played by temperature in the atmospheric corrosion of steel What is the effect of wind velocity, thermal capacity of the metal and its insulation properties on temperature ... [Pg.574]

These properties of water have important consequences in its role in the ecosystem of Earth. Water at a temperature of 4 °C will always accumulate at the bottom of fresh water lakes, irrespective of the temperature in the atmosphere. Since water and ice are poor conductors of heat (good insulators) it is unlikely that sufficiently deep lakes will freeze completely, unless stirred by strong currents that mix cooler and warmer water and accelerate the cooling. In warming weather, chunks of ice float, rather than sink to the bottom where they might melt extremely slowly. These phenomena thus may help to preserve aquatic life. [Pg.86]

Thermal escape, Jeans escape if we assume that the individual molecules are Maxwellian distributed, then molecules from the high tail of this distribution can escape, if at a given level in the atmosphere the mean free path is comparable to the scale height. According to Maxwell s distribution, the kinetic energy of the molecules depends on the mass and velocity (which depends on the temperature in the atmosphere) ... [Pg.143]


See other pages where Temperature in the atmosphere is mentioned: [Pg.293]    [Pg.283]    [Pg.955]    [Pg.403]    [Pg.214]    [Pg.181]    [Pg.94]    [Pg.81]    [Pg.77]    [Pg.223]    [Pg.77]    [Pg.169]    [Pg.293]    [Pg.8]    [Pg.11]    [Pg.11]    [Pg.466]    [Pg.8]    [Pg.463]    [Pg.31]    [Pg.4]    [Pg.988]    [Pg.224]   
See also in sourсe #XX -- [ Pg.161 ]




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