487 research outputs found
Measurement of NO plus plus e minus dissociative recombination in expanding air flows
Measurement of nitric oxide ion-electron dissociative recombination in expanding air flow
Sources of electron energy in weakly ionized expansions of nitrogen
Sources of electron energy in weakly ionized expansions of nitroge
Catalysis of hydrogen-atom recombination in rocket nozzles
Oxygen and oxygen-nitrogen mixtures as catalysts for hydrogen atom recombination in rocket nozzle
Characteristics of the motions, turbulence intensity, diffusivity, flux of momentum and sensible heat in the upper atmosphere
Analyses of the meteorological rocket data obtained from an experiment conducted at 3-hour intervals at 8 western meridional rocket stations are presented. Large variations in the meridional wind contribute substantially to overall turbulence in the tropical stratosphere. The solar semidiurnal component of wind oscillations in the tropics was observed to be much higher than predicted by theory, often exceeding the magnitude of the diurnal amplitude throughout the stratosphere. The observed value of the solar diurnal amplitude in the stratosphere was in line with theoretical prediction. The solar terdiurnal amplitudes for temperature, meridional and zonal winds were non-negligible and must be considered in any harmonic analysis. Phase angle variation with height was rapid for all harmonics; however, there was general agreement between predicted and observed phase angles. Because of large changes in the mean winds in the mesosphere with season, harmonic determinations are difficult. There appear to be large zonal wind changes even within the same season as mentioned previously. Turbulence diffusivity in the upper stratosphere is greater near the equator than in the mid-latitudes
Globalized World and Separation of Powers: A New Role for the Independent Administrative Authorities
- …