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  • 1
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    Diurnal variations of odd nitrogen and ionic densities in the mesosphere and lower thermosphere - Simultaneous solution of photochemical-diffusive equations (1975)
    In:  Other Sources
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    Publication Date: 2011-08-16
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 80; Oct. 1
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  • 2
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    Thermal structure of the primitive ionosphere (1978)
    In:  Other Sources
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    Publication Date: 2011-08-17
    Description: Exospheric neutral and electron temperatures have been estimated for the primitive upper atmosphere and ionosphere with various oxygen content in the scheme of our previous model (Shimizu and Shimazaki, 1976). The exospheric neutral temperature has been shown to be rather insensitive to the change of oxygen content, justifying our previous assumption for the temperature variation, while the exospheric electron temperature has been found to be quite sensitive to the compositional change, mainly owing to the strong dependence of electron density on the oxygen concentration.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 83; Jan. 1
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  • 3
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    The photochemical time constants of minor constituents and their families in the middle atmosphere (1984)
    In:  Other Sources
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    Publication Date: 2011-08-18
    Description: A comprehensive formula is worked out for the photochemical time constant of minor constituents in the middle atmosphere. The formula is particularly useful for evaluating the time constants for families of some chemical species that are strongly coupled by rapid exchange reactions. Height profiles of photochemical time constants are calculated for individual species and their families based on the chemical reaction rate constants recommended in the recent WMO and JPL reports. Potential exchange reactions among various family members are discussed, and the effects of the choice of family membership on the time constant are evaluated.
    Keywords: GEOPHYSICS
    Type: Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169); 46; 173-191
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  • 4
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    The dayside Venus ionosphere. II - Combined numerical model of ion and neutral composition above 120 km (1984)
    In:  Other Sources
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    Publication Date: 2011-08-19
    Description: The median vertical profile of ion densities for the dayside Venusian ionosphere obtained by the orbiter retarding potential analyzer (ORPA) is simulated by one-dimensional model calculations. The model includes both neutral and ionic chemistry, eddy and molecular diffusion for neutral constituents, and ion-plasma diffusion for ionic constituents. The electron and ion temperatures measured by the ORPA are used to calculate the plasma diffusion coefficients and scale heights for ions. The predicted O2(+) densities below about 200 km agree particularly well with observations by the ORPA, but the model values are significantly less than those measured by the orbiter ion mass spectrometer. The observed ion composition is interpreted in terms of densities of the neutral atmosphere and its composition.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Icarus (ISSN 0019-1035); 60; 654-674
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  • 5
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    A model of temporal variations in ozone density in the Martian atmosphere (1981)
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    Publication Date: 2011-08-18
    Description: Temporal variations of the ozone density profile in the Martian atmosphere at high latitudes are calculated for the course of a Martian year, taking into account seasonal and diurnal variations in temperature, water vapor and solar radiation. Calculations are based on a model including 35 neutral photochemical reactions, and vertical eddy diffusion using a time step of 12 min for the region from the surface to 240 km altitude. Results are found to be in better agreement with Mariner 9 observations of the time and magnitude of the seasonal maximum than previous model calculations. The diurnal variation is predicted to be small near the solstices, with the nighttime ozone density greater than the daytime and the magnitude of the difference dependent on season. Opposite temporal variations are predicted for ozone densities above and below about 25 km, and an ozone density maximum at 35-40 km is obtained. It is suggested that the effects of an aerosol layer may not be important in enhancing predicted ozone concentration, and may even decrease it.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Planetary and Space Science; 29; Jan. 198
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  • 6
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    Evolution of the ionosphere (1976)
    In:  Other Sources
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    Publication Date: 2011-08-16
    Description: Studies were made of the electron density profiles at various stages of atmospheric evolution, with the assumption that the atmospheric composition has changed due to the gradual increase of oxygen while the nitrogen level has remained constant. The result of model calculations indicates that when the oxygen content is less than about 1% of the present earth's atmosphere level, the major ions in the F2 region will change from O(+) to N(+). The maximum number density of N(+) ions reaches approximately 10 million per cu cm because of the absence of a rapid loss mechanism for N(+). The height of the N(+) ion density peak is much lower than the height of the F2 layer peak of the current ionosphere.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 81; Sept. 1
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  • 7
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    A comparison of one-dimensional theoretical models of stratospheric minor constituents (1976)
    In:  Other Sources
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    Publication Date: 2011-08-16
    Description: The density profiles of stratospheric minor constituents are compiled from several one-dimensional theoretical models that have appeared in the literature. The models are compared with each other and also with observations if data are available. The similarity and disparity of the models are clarified and discussed. If a large difference exists among the models, attempts are made to interpret it as much as possible in terms of the physical and chemical data employed in each model. The inadequacy of one-dimensional models in calculating the realistic ozone density distributions and the problems related to it are briefly discussed.
    Keywords: GEOPHYSICS
    Type: Reviews of Geophysics and Space Physics; 14; Feb. 197
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  • 8
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    The seasonal variation of ozone density in the Martian atmosphere (1979)
    In:  Other Sources
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    Publication Date: 2011-08-17
    Description: A one-dimensional, time-dependent model has been developed to investigate seasonal variations in ozone density in the Martian atmosphere. The model utilizes data for atmospheric temperature, pressure, and water vapor abundance observed by Viking. The results indicate that a high ozone density is not produced near the winter solstice but is in rather late winter, when the amount of water vapor is still small and the solar radiation can penetrate more deeply. A similar condition met in early winter does not necessarily produce a high ozone density because of the predicted higher HO2 density. Seasonal variations in ozone abundance are discussed in terms of the abundances of H2O and H2 and the seasonal variations in their reaction products H2O2 and HOx. The roles of transport, the effects of ozone loss to the surface, and the differences between northern and southern hemisphere ozone distributions are also discussed.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Journal of Geophysical Research; 84; Apr. 1
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  • 9
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    Radiative relaxation of molecular vibration of the nitric oxide molecule as a possible source of the infrared Shuttle glow (1985)
    In:  Other Sources
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    Publication Date: 2011-08-19
    Description: A model calculation to predict infrared Shuttle flow due to the radiative relaxation of vibration of the NO molecule is presented. Space Shuttles hit atmospheric NO molecules at a very high speed and excite vibrational and rotational motions up to the temperature of 54,000 K. With the electric dipole radiation of delta v = 1, 2, 3, and particularly 4 (v is the vibrational quantum number), the excited NO molecules emit infrared radiation before they collide with other molecules. The total radiation power is estimated to be 170 A micro-W, where A is the cross-section area of the Shuttle in sq m if no adsorption of the NO molecule takes place on the Shuttle surface. The intensity of each infrared line is calculated as a function of time, including all vibrational states up to v = 35.
    Keywords: SPACECRAFT DESIGN, TESTING AND PERFORMANCE
    Type: Planetary and Space Science (ISSN 0032-0633); 33; 1119-112
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  • 10
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    Nighttime variations of F-region electron density profiles at Puerto Rico. II - An attempt to separate the effects of temperature variation and drift velocity. (1966)
    In:  Other Sources
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    Publication Date: 2019-05-30
    Description: Temporal variations in temperature and drift velocity in ionosphere determined from nighttime variations of F-region electron density profiles at Puerto Rico
    Keywords: GEOPHYSICS
    Type: JOURNAL OF GEOPHYSICAL RESEARCH
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