Involutional matrices based on the representation theory of GL/2/.
Mathematical properties of involutional matrix solutions to simple quadratic equation, obtaining symmetry properties, eigenvalues and recursion formulas
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Mathematical properties of involutional matrix solutions to simple quadratic equation, obtaining symmetry properties, eigenvalues and recursion formulas
Unitary matrix representing generalized inverses, proving weak method of steepest descent for least squares solution of equations
Orbit calculation by fitting functions to osculating orbital elements
Integral equation for emissivity inside uniform gray isothermal Lambertian cavity solved using successive approximations
Poisson shot noise process relationship with continuous stochastic intensity as sample function
Frequency domain analogies, polynomial matrices, and linear systems
Flow equation for representing ion beam current density profile from bombardment ion thrusters
Calculation of power scattered by large, homogeneous body bounded by smooth, undulated surface when illuminated by incident field of finite extent - Vol. 2
Analysis, synthesis, and transmission of human speech based on computation of time intervals between threshold transitions of speech waveform derivatives
Nonstationary colored noise linear shaping filter to transform white noise into nonstationary random process with specified covariance function
Our method of matrix synthesis of optical components and instruments is applied to the derivation of Jones's matrices appropriate for Fourier interferometers (spectrometers and spectropolarimeters). These matrices are obtained for both the source beam and the detector beam. In the course of synthesis, Jones's matrices of the various reflectors (plane mirrors; retroreflectors: roofed mirror, trihedral and prism cube corner, cat's eye) used by these interferometers are also obtained.
A program to integrate the equations of motion by series in powers of the time step can be easily modified to furnish the elements of the matrizant in power series of the time step. In particular, if the series representing the motion are obtained recursively, differentiation of the recurrence relations will provide immediately a recursive scheme for computing the coefficient in the power series for the elements of the matrizant.
The paper represents the earth's gravitational potential V, outside a sphere bounding the earth, by means of its difference from the author's spheroidal potential. The difference is in turn represented as arising from a surface density on the sphere bounding the earth. Because of the slow decrease with order n of the normalized coefficients in the spherical harmonic expansion of V, the density anomalies from which the higher coefficients arise must occur in regions close to the earth's surface. The surface density is thus an idealization of the product of the density anomaly and the crustal thickness. Values of surface density are computed from potential coefficients obtained from two sources, Rapp and the Smithsonian Astrophysical Observatory. The two sources give qualitative agreement for the values of surface density and for its contour map. The numerical values obtained for surface density are compatible with the idea that the responsible density anomalies are reasonably small, i.e., less than 0.05 g/cu cm, and occur in the crust alone.
A basic description is given of the mathematical tools and models which are presently used to represent turbulent, free shear layers. Recommendations are included for ways in which current modeling techniques can be improved.
An explanation is presented of the method used to locate the elastic axis and the method to determine the EI and GJ distributions along the elastic axes of wings with a 2-spar (front and rear) construction or a single torque-box construction.
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