Results 241 to 250 of about 2,078,180 (298)
Concurrent tunable structural color, luminescence, and afterglow in single ZnS: X@SiO2 spheres via SiO<sub>2</sub>-nanoarmor and calcination decoupling collaborative strategy. [PDF]
Smart MolLiu T, Meng R, Zhang S, Wu S.
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Fractional Ion Contributions to Mixed Electrolyte Ion Atmospheres from Experimental Thermodynamic Data. [PDF]
J Phys Chem BPloetz EA, Smith PE.
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Effects of Ambient Oxygen Concentration on Microstructural Evolution and Mechanical Properties of Wire Arc Additively Manufactured Ti-6Al-4V Thin-Walled Components. [PDF]
Materials (Basel)Meng S +6 more
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Latitudinal manganese gradient dynamics associated with Earth's major ice ages. [PDF]
Nat CommunWang X, Pohl A, Rickaby REM, Lu Z.
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Science, 1966
The thermal structure of the upper atmosphere of Mars has been theoretically investigated. The exospheric temperature, for a pure CO 2 model atmosphere, lies between 400° and 700°K. The origin of the Martian atmosphere is discussed in the light of these results.
S H, Gross, W E, McGovern, S I, Rasool
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The thermal structure of the upper atmosphere of Mars has been theoretically investigated. The exospheric temperature, for a pure CO 2 model atmosphere, lies between 400° and 700°K. The origin of the Martian atmosphere is discussed in the light of these results.
S H, Gross, W E, McGovern, S I, Rasool
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Ionisation in the Upper Atmosphere
Nature, 1927THE more important agencies which may conceivably cause the ionisation of the upper atmosphere of the earth are the ultra-violet light, α- and β-particles, all of solar origin, the penetrating radiation of cosmic origin, and the ionising radiations from terrestrial sources.
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Upper atmospheric nomenclature
Journal of Atmospheric and Terrestrial Physics, 1950It is proposed that stratosphere shall signify solely the nearly isothermal region above the troposphere; that the layer between the stratosphere and the deep temperature minimum somewhat below 100 km be called the mesosphere; that the layer of rising temperature over this minimum be called the thermosphere.
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Terrestrial Magnetism and Atmospheric Electricity, 1928
The density calculations of the following paragraphs are based on the assumptions of diffusion as indicated by Table 3 and temperature‐distribution as shown in Figure 7. The calculations for the atmospheric conditions of summer nights are given in detail since it was considered these figures would be the most useful.The change in atmospheric pressure ...
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The density calculations of the following paragraphs are based on the assumptions of diffusion as indicated by Table 3 and temperature‐distribution as shown in Figure 7. The calculations for the atmospheric conditions of summer nights are given in detail since it was considered these figures would be the most useful.The change in atmospheric pressure ...
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1990
Under the powerful ultraviolet radiation from the sun the higher and thinner layers of the atmosphere become ionized and produce important consequences for the propagation of radio waves. More generally, because of the large mean free paths the medium is not in thermal equilibrium and many complex atomic and molecular phenomena take place.
Bruno Bertotti, Paolo Farinella
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Under the powerful ultraviolet radiation from the sun the higher and thinner layers of the atmosphere become ionized and produce important consequences for the propagation of radio waves. More generally, because of the large mean free paths the medium is not in thermal equilibrium and many complex atomic and molecular phenomena take place.
Bruno Bertotti, Paolo Farinella
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2011
Conditions in the outermost region of the atmosphere differ radically from those in the lower atmosphere. The principal characteristic features are the following:
Peter Warneck, Jonathan Williams
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Conditions in the outermost region of the atmosphere differ radically from those in the lower atmosphere. The principal characteristic features are the following:
Peter Warneck, Jonathan Williams
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