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The Earths Atmosphere

The bottom layer of air in the troposphere, that 1 to 2 km of air closest to the earth s surface, can be called the atmospheric boundary layer. From the point of view of atmospheric chemistry, four regions of the atmospheric boundary layer can be identified  [Pg.327]

the urban atmosphere—the region most strongly influenced by anthropogenic emissions [Pg.327]

the regional atmosphere—a region influenced by both anthropogenic and natural emissions [Pg.327]

the remote, tropical forest atmosphere—a region essentially free of anthropogenic emissions but strongly influenced by natural biogenic emissions [Pg.327]

Typical Ozone and NO Mixing Ratios in Regions of the Troposphere [Pg.328]


Pollution, n the action of polluting the condition of being polluted. Pollute, vt [L. pollutus, past part, or polluere, to make physically impure or unclean] to defile, desecrate, profane-syn. see CONTAMINATE. Air, n [fr. L aer, fr. Gr. aer] 1. the mixture of invisible tasteless gases which surrounds the earth. Atmosphere, n [fr. Gr. (atmo and sphaira) 2. the whole mass of air surrounding the earth. . . ... [Pg.19]

Using Wien s displacement law, determine the mean effective temperature of the earth-atmosphere system if the resulting longwave radiation peaks at 11 /rm. Contrast the magnitude of the radiant flux at 11 pm with that at 50 pm. [Pg.273]

Very light gases, notably hydrogen and helium, tend to escape from the earths atmosphere. The hydrogen you generate in the laboratory today is well on its way into outer space tomorrow. A similar situation holds with helium, which is found in very limited quantities mixed with natural gas in wells below the earths surface. If helium is allowed to escape, it is gone forevei and our supply of this very usefiil gaseous element is depleted. [Pg.111]

Infrared optics is a fast growing area in which CVD plays a maj or role, particularly in the manufacture of optical IR windows. 1 The earths atmosphere absorbs much of the infrared radiation but possesses three important bandpasses (wavelengths where the transmission is high) at 1-3 im, 3-5 im and 8-17 pm. As shown in Table 16.2, only three materials can transmit in all these three bandpasses single crystal diamond, germanium, and zinc selenide. [Pg.414]

Abstract This is a tutorial about the main optical properties of the Earth atmosphere as it affects incoming radiation from astrophysical sources. Turbulence is a random process, of which statitical moments are described relying on the Kolmogorov model. The phase structure function and the Fried parameter ro are introduced. Analytical expressions of the degradation of the optical transfer function due to the turbulence, and the resulting Strehl ratio and anisoplanatism are derived. [Pg.1]

Hence, the radiative equilibrium temperature is sensitive to changes in the solar constant, planetary albedo, and the radiative properties of the earth-atmosphere-ocean system. In addition, changes internal to the earth-atmosphere-ocean system may alter the climate. Table I is an incomplete list of phenomena that individually or in concert could alter climate. [Pg.386]

Figure 2. Within the Earth-atmosphere system numerous feedback loops govern climate. (Reproduced with permission from ref. 31. Copyright 1974 American Association for the Advancement of Science.)... Figure 2. Within the Earth-atmosphere system numerous feedback loops govern climate. (Reproduced with permission from ref. 31. Copyright 1974 American Association for the Advancement of Science.)...
Occurrence. Naturally occurring nitrogen (N2) makes up 78% (by volume) of the earth atmosphere. Nitrogen is relatively unabundant in the crustal rocks. The major minerals are saltpetre (KN03) andNaN03 (Chile saltpetre). [Pg.507]

Oxygen is the third most abundant element in the universe, making up nearly half the mass of the Earths crust and nine-tenths of the total mass of water. Even the mass of our bodies consists of two-thirds oxygen. Oxygen is also the most abundant element in the Earths atmosphere at 20.947% by volume. [Pg.226]

Argon is a colorless, odorless, tasteless, chemically inert noble gas that makes up about 0.93% of the Earths atmosphere. It is the third most abundant gas in the atmosphere, meaning it is more common than carbon dioxide, helium, methane, and hydrogen. [Pg.267]

It is important to emphasize that because the greenhouse effect originates in radiative transfer processes in the earth-atmosphere system, the net effect of a... [Pg.769]

Bombs, Atomie, See Atomic(or Nuclear) Bomb in Vol l,p A499-L. Explosion of atomic bomb in the earth atmosphere was discussed by H.Schwentek,... [Pg.238]

Assessment and prediction needs for the earth-atmosphere system... [Pg.302]

In addition to the transition phenomena mentioned so far in the present section, a variety of even larger scale processes might have operated during chemical evolution, namely, instabilities and bifurcations in the very atmospheric environment within which life emerged. As shown in the paper by Marcel Nicolet, the earth s atmosphere is the theater of a variety of complex chemical and transport phenomena. Moreover, as explained by Stanley L. Miller, the composition of the primordial atmosphere has certainly affected deeply the chemistry in the primitive oceans. Conversely, once life emerged the properties of the atmosphere changed radically, and this must have affected the further course of evolution. We refer to Prather et al.41 and North et al.42 for an account of present views on large scale transitions in the earth-atmosphere system. [Pg.191]

Some molecules in this group (HONO, NC j 0, HONC ) have been extensively studied because the photofragments OH and NO can be probed by tunable lasers. These molecules are important minor constituents in the earth atmosphere and their photochemistry plays a major role in air pollution. Atmospheric pollutants N0X (NO, NO2, NO3) are formed from combustion of fuel and subsequent chemical reactions in the atmosphere. Photolysis of alkyl oxides produces NO and NO2 that can be probed by LIF the internal energy distribution provides an important clue to the mechanism of photodissociation. [Pg.23]

Some halogen compounds have been too reactive for the health of people and the planet. They can destroy healthy cells and attack the Earths atmosphere in the same active way that they kill germs or break down wood into paper. For instance, chlorofluorocarbon (or CFC) compounds used to be popular cooling chemicals in refrigerators and air conditioners and in the gas that pushed hairspray and deodorant out of aerosol cans. CFCs are now widely banned because they destroy Earths atmosphere. Chlorine is also part of the insect killer DDT, a dry cleaning fluid, and the compounds called PCBs. All of these products are now banned or used rarely because they have been linked to pollution and health problems like cancer and liver disease. [Pg.81]

ADEOS An improved, satellite Earth-observing system equipped with modernized radiometer of the visible and near-IR intervals (AYNIR), ocean color and temperature scanner (OCTS), and radiometer POLDER to carry out global systematic measurements of polarization and spectral characteristics of solar radiation reflected by the Earth-atmosphere system. The satellite ADEOS-2/ Midori-2 was launched on December 14, 2002 by the Japan Space Agency and is an ideal means of global monitoring. [Pg.293]

Tal rose [23] and many other authors [24, 25] presented an interesting sphere of HO radical participation non-linear reactions and ozonosphere processes proceeding at ozone formation in the Earth atmosphere and chemical lasers. [Pg.151]

Figure 7.1 shows a noble gas elemental abundance relative to 36Ar for the Earth atmosphere, Q, SW, and lunar soils [cf. Table 3.2,3.3(a), and 3.3(b)]. We also included the supposed Martian atmospheric noble gas (e.g., Pepin, 1991). The abundances are normalized to the solar (cosmic) abundance. [Pg.220]

Marty, B. (1989) Neon and xenon isotopes in MORB Implications for the earth-atmosphere evolution. Earth Planet. Sci. Lett., 94, 45-56. [Pg.266]

Ozima, M., Alexander, Jr., E. C. (1976) Rare gas fractionation patterns in terrestrial samples and the earth-atmosphere evolution model. Rev. Geophys. Space Phys., 14, 385-90. [Pg.270]

Any other body which has absorptivity a fiw) = 1 for photons with energy Hui will emit radiation according to (4.1). Although the sun consists mainly of protons, alpha particles and electrons, its absorptivity is a(Tkj) = 1 for all photon energies tiw, by virtue of its enormous size. Its temperature is not homogeneous, but emitted photons originate from a relatively thin surface layer a few hundred kilometres thick, in which the temperature is constant and in which all incident photons are absorbed. Conversely, only photons emitted within this surface layer may reach the surface of the sun. The solar spectrum observed just outside the Earth atmosphere agrees well with (4.1)... [Pg.118]

AM (0) sunlight The solar irradiance in space just above the earth atmosphere (air mass, AM, zero). Also called extraterrestrial global irradiance. [Pg.301]


See other pages where The Earths Atmosphere is mentioned: [Pg.621]    [Pg.379]    [Pg.380]    [Pg.383]    [Pg.386]    [Pg.390]    [Pg.71]    [Pg.114]    [Pg.2]    [Pg.194]    [Pg.233]    [Pg.51]    [Pg.282]    [Pg.763]    [Pg.162]    [Pg.162]    [Pg.162]    [Pg.166]    [Pg.1006]    [Pg.3]    [Pg.108]    [Pg.80]    [Pg.464]    [Pg.419]    [Pg.420]    [Pg.42]    [Pg.284]    [Pg.11]   


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Earth atmosphere

Earth atmospheric

THE EARTH

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