The inclined incidence of gamma-ray
Buildup dose factors with inclined incident gamma radiations, for radiation shielding design
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Buildup dose factors with inclined incident gamma radiations, for radiation shielding design
Satellite motion for all inclinations around oblate planet with potential including second and fourth zonal harmonics
Preliminary analysis of three impulse technique for transearth injection from highly inclined orbits
Instability of inclined stiffened thin circular cylindrical shells under pure bending using Ritz method
Optimal fixed time N impulse trajectory determination between inclined orbits using primer vector theory method
Improved coefficients of thirteenth order harmonics of geopotential derived from satellite Doppler data at three orbital inclinations
Theoretical shape of magnetosphere boundary considering inclination of geomagnetic dipole and nondipole part of geomagnetic field
Transient condensing with freezing on nonisothermal inclined plate
Discharge nozzle coefficients for thick plate orifices with approach flow perpendicular and inclined to orifice axis
Characteristics method for determining three dimensional supersonic flow around inclined body of revolution
Inclination effect of fatigue cracks on plane strain fracture toughness of 7075-T651 Al alloy, discussing cantilever bending
Film cooling following air injection through inclined flat plate holes into turbulent boundary layer
Stiffener inclination effect on pressurized cylinder instability under pure bending
Stiffeners inclination effects on instability of pressurized cylinder under bending by Ritz method, considering finite deflection and initial imperfections in strain-displacement relations
Liquid oscillation frequency measurement in inclined right circular cylinder
General relativistic precession of gyroscope in inclined orbit
Geomagnetic field inclination determination by incoherently scattered signal Faraday rotation calibration and simultaneous ionosonde measurements of ionospheric electron density
Careful re-measurement of all available plates showing Uranus V (Miranda), supplemented by some recently obtained images, shows that this satellite has both a pronounced orbital eccentricity and inclination (to the plane of the other satellites). Observations are sufficient in number and distribution to allow determinations of the precession rates of both pericenter and node, with implications for the dynamical oblateness of Uranus and the gravitational interaction of the satellites. An improved value for the revolution period is a byproduct of the investigation. The success of the study is due to the improved precision of the measures resulting from the adoption of a very simple, direct method of measurement.