Heterogeneous Integrated Failure Analysis Using Radio Frequency Signal Detection/Injection with Power Spectrum Analysis
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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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Low rigidity cosmic ray modulation and interplanetary medium at solar minimum and at other phases of solar cycle
Stellar scintillation spectra theory extended to rectangular apertures, generalizing to planetary scintillation and effects of diffraction, atmospheric dispersion and seeing
Randomly fluctuating, non-Gaussian pressure gradient effect on steady, incompressible channel flow
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It is shown here that, by using galaxy catalog correlation data as input, measurements of microwave background radiation (MBR) anisotropies should soon be able to test two of the inflationary scenario's most basic predictions: (1) that the primordial density fluctuations produced were scale-invariant and (2) that the universe is flat. They should also be able to detect anisotropies of large-scale structure formed by gravitational evolution of density fluctuations present at the last scattering epoch. Computations of MBR anisotropies corresponding to the minimum of the large-scale variance of the MBR anisotropy are presented which favor an open universe with P(k) significantly different from the Harrison-Zeldovich spectrum predicted by most inflationary models.
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Interstellar scintillation (ISS), fluctuations in the amplitude and phase of radio waves caused by scattering in the interstellar medium, is important as a diagnostic of interstellar plasma turbulence. ISS is also of interest because it is noise for other radio astronomical observations.
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