A Class of Related Space-times
Relationship of Riemannian space-times with metric tensors in solution of vacuum field equations
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Relationship of Riemannian space-times with metric tensors in solution of vacuum field equations
Space time distribution of solar cosmic rays in interplanetary space
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Measurements of the statistical properties of the fluctuating wall pressure produced by a subsonic turbulent boundary layer are described. The measurements provide additional information about the structure of the turbulent boundary layer; they are applicable to the problems of boundary-layer induced noise inside an airplane fuselage and to the generation of waves-on water. The spectrum of the wall pressure is presented in dimensionless form. The ratio of the root-mean-square wall pressure to the free-stream dynamic pressure is found to be a constant square root of bar P(sup 2)/q(sub infinity) = 0.006 independent of Mach number and Reynolds number. In addition, space- time correlation measurements in the stream direction show that pressure fluctuations whose scale is greater than or equal to 0.3 times the boundary-layer thickness are convected with the convection speed U(sub c) = 0.82U(sub infinity) where U(infinity) is the free-stream velocity and have lost their identity in a distance approximately equal to 10 boundary-layer thicknesses.
A radiometric consistent climate fingerprinting methodology has been developed to derive long-term temperature, water vapor, cloud, trace gases, and surface skin temperature anomaly time series from the hyper-spectral sounder measurements of multiple platforms. The spectral fingerprinting methodology requires the use of radiative kernels that are radiometrically consistent with observations. Radiative kernels are built using space-time averaged Jacobians that are physically retrieved from observations under all sky conditions. The physical retrieval algorithm uses the Principal Component based Radiative Transfer Model (PCRTM) for the forward simulation. The incorporation of multiple scattering simulation in PCRTM allows the direct radiative relationship between single field-of-view (FOV) radiance observations and corresponding thermal dynamic variables including cloud properties to be established. Therefore, radiance ?closure? can be achieved under all-sky conditions by the fingerprinting scheme. This methodology has been used to derive climate anomalies from the space-time averaged spectra of AIRS/AMSU and CrIS/ATMS. The use of a consistent fingerprinting scheme provides an effective mean of generating continuity product by merging observations from different platforms and therefore facilitating the long-term climate trend study.
General covariance principle for operation and measurement requirements of space-time models
Connection between internal and space-time symmetries in high energy interactions - theoretical physics
Group-theoretical method for internal symmetries of elementary particles from space-time geometry determination
Proposed units of length and time to facilitate coordination of space-time positions in orbital operations
Solution of Einstein field equations with incoherent matter for homogeneous space-time case using spinor technique, including Goedel theorem proof
Homogeneous solution of Einstein-Maxwell equations assuming invariant space-time metric and electromagnetic field
Theory of fundamental particle symmetries derived from basic properties of space-time using principles of quantum mechanics and special relativity
Covariance groups and role of space-time coordinates in relativity theory
Interaction energy in geometrostatics - geometrodynamic description of particles by topological features of empty space-time
Space-time temperature distribution in one- dimensional systems with heat transfer across contacts
Evaluation of general physical condition of Gemini IV flight crew with increasing time under space flight conditions - response of cardiovascular system to calibrated workload
Euclidean nature of relativistic rotating disk in conclusions of Eddington and Lorentz