Nonlinear spin-wave theory for the anisotropic Heisenberg antiferromagnet
Nonlinear spin wave theory for anisotropic antiferromagnetism, solving sublattice magnetization by thermodynamic Green function for temperature dependence
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Nonlinear spin wave theory for anisotropic antiferromagnetism, solving sublattice magnetization by thermodynamic Green function for temperature dependence
Anisotropic solar cosmic rays in inhomogeneous medium, investigating shell effect on propagation by one dimensional model
Anisotropic superconducting energy gap of pure Zn from microwave absorption measurements
Anisotropic energy gap model in superconducting Zn to describe microwave absorption measurements
Anisotropic multifluid cosmological models with orthogonal velocity fields
Dipole antenna radiation in compressible anisotropic electron plasma overlying imperfectly conducting half space, solving for lunar environment
Dipole antenna radiation in compressible anisotropic electron plasma overlying imperfectly conducting half space, evaluating Fourier- Bessel integrals for lunar environment
Anisotropic Heisenberg antiferromagnet theory, developing nonlinear spin-wave approximation
Omnidirectional anisotropic molecular trap, used with vacuum pump to simulate space environments for testing spacecraft components
Radio wave scattering from random electron density fluctuations in cold anisotropic magnetoplasma
Buckling of boron/aluminum and graphite/resin fiber composite anisotropic panels - load tests
Stress waves induced in anisotropic fiber composite plates by transverse, short-duration impact forces
Two fluid model of solar wind with anisotropic proton temperature and allowing for extended coronal proton heating
Anisotropic Heisenberg antiferromagnet sublattice magnetization, obtaining temperature dependence
Theoretical results are presented for the buckling of anisotropic plates. The plates are subjected to simple and combined in-plane loading. The plates are made from fiber composite material of boron/aluminum or high-modulus graphite/resin. The results are presented in nondimensional form as buckling load against fiber orientation angle for various plate aspect ratios. The results indicate that buckling loads of boron/aluminum plates are independent of fiber direction if the plate aspect ratios are greater than about 1, and moderately dependent when this ratio is less than about 1. In addition, the results indicate that the buckling loads are independent of aspect ratio for plates with aspect ratios greater than about 2. Boron/ aluminum composite plates can resist buckling loads more efficiently than graphite/resin composites on a specific buckling stress basis. The numerical algorithm and a listing of the computer code used to obtain the results are included.
Theoretical results are presented for the buckling of anisotropic plates. The plates are subjected to simple and combined inplane loading. The plates are made from fiber composite material of boron/aluminum or high modulus graphite/resin. The results are presented in nondimensional form as buckling load vs fiber orientation angle for various plate aspect ratios.
The dispersion equation is obtained analytically of waves along an infinitely long cylindrical ?grid-like' antenna in an anisotropic compressible homogeneous plasma. Numerical solutions of this equation show that an external static magnetic field has great influence upon the anomalously dispersive region of the dispersion relation around the plasma frequency.
At times, the electron pitch angle distributions at synchronous orbit have been observed to be highly anisotropic. In the local morning region, distributions concentrated near 90 deg are often observed in particles of less than approximately 2000 V. This anisotropy decreases with increasing energy from 1 keV to the detector's limit at 50 keV. The time development of anisotropy is consistent with production by pitch angle scattering processes which are not effective on electrons with small velocities parallel to the magnetic field. Another type of distribution has been observed with the low-energy (below 1000 V) electrons concentrated parallel and antiparallel to the magnetic field. These distributions are only seen in the dusk sector, but this may be an orbital artifact.