THEORETICAL MODELS FOR THE SOLAR-CYCLE VARIATION OF THE UPPER ATMOSPHERE
Theoretical models for solar-cycle variation of upper atmosphere
SOLAR CYCLE↗
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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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THEORETICAL ESTIMATES OF THE AVERAGE SURFACE TEMPERATURE ON MARS
Theoretical estimates of average surface temperature of mars by use of greenhouse model
PLANETARY ATMOSPHERE↗
THEORETICAL TIDES ON A RIGID, SPHERICAL MOON
Theoretical tidal tilts and changes in gravitational acceleration make possible the determination of gross physical properties of the moon
GRAVITATIONAL EFFECT↗
THEORETICAL AND EXPERIMENTAL MODELS FOR UNSTABLE ROCKET COMBUSTOR
Theoretical and experimental models of the study of combustion instability in rocket combustors
ROCKET COMBUSTOR↗
RELATION BETWEEN THEORETICAL AND OBSERVATIONAL MODELS OF THE UPPER ATMOSPHERE
Solar cycle variations of upper atmospheric properties, comparing air density observations with theoretical models
UPPER ATMOSPHERE↗
Problems of theoretical seismology and physics of the earth's interior <voprosy teoreticheskoi seismologii i fiziki zemnykh nedr<
Theoretical seismology and physics of earth core and mantle
SEISMOLOGY↗
Theoretical estimates of the average surface temperature on mars
Estimates of the average surface temperature on Mars are derived from radiative equilibrium considerations. A minimum possible surface temperature is estimated by computing the radiative equilibrium temperature that the Martian surface would have if the planet had no atmosphere. An estimate of the maximum possible value of the average surface temperature is obtained by computing the surface temperature that would result from a maximum greenhouse model. The computations indicate that the average surface temperature is in the range 219K to 233K. Comparisons of the theoretical computations with indications of surface temperature obtained from thermal emission observations are found to be in reasonable agreement.
Surface temperature↗
A theoretical study of the martian ionosphere.
Theoretical study of martian ionosphere for analyzing the feasibility of rocket exploration of the planet
IONOSPHERIC SOUNDING↗
Thin-film thickness from theoretical expressions for conductivity and isothermal Hall effect.
Thin film thickness from theoretical expressions for conductivity and isothermal Hall effect
THIN FILMS↗
Theoretical Stability Derivatives for the X-15 Research Airplane at Supersonic and Hypersonic Speeds Including a Comparison with Wind-tunnel Results
Longitudinal and lateral stability and control derivatives for X-15A aircraft at supersonic and hypersonic speeds - comparison of theoretical results with wind tunnel testing
LATERAL STABILITY AND CONTROL↗
Relation between theoretical and observational models of the upper atmosphere
Relation between theoretical and observational models of atmospheric properties and changes during decreasing solar activity
CELESTIAL OBSERVATION↗
Theoretical study of non-equilibrium ioniza- tion in the presence of electric and magnetic fields progress report no. 3, 1 feb. - 31 jul. 1964
Theoretical study of nonequilibrium ionization in presence of electric and magnetic fields
MAGNETIC FIELD↗
A theoretical investigation of the rolling motion of the nike cajun and nike apache rocket vehicles
Theoretical prediction of rolling motion of Nike-Cajun and Nike-Apache rocket vehicles
NIKE-CAJUN ROCKET↗
Theoretical basis of the jpl orbit determina- tion program
Theoretical basis of orbit determination - mathematical model, computation and correction of observables, and regression coefficients
REGRESSION COEFFICIENT↗
Theoretical and experimental investigation of an unsteady vortex flow <theoretische und experimentelle untersuchungen an einer instationaeren wirbelstroemung<.
Unsteady vortex flow about vertical wedge in shock tube studied by interferometric and theoretical method
SHOCK TUNNEL↗
Theoretical line profiles in the ultraviolet spectra of early-type stars.
Theoretical line profiles in UV spectra of two early B stars from 911.6 to 3000 angstroms
STELLAR SPECTRUM↗
Theoretical interpretation of tait equation parameters.
Tait parameters relation to theoretical equation of state
THERMODYNAMIC PROPERTY↗
Theoretical curves of backscattering cross sections of rough surfaces for several polarization states using two statistical models
Theoretical curves of backscattering cross sections of rough surfaces for polarization states using statistical models
BACKSCATTER↗