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Mathematical Analysis of Random Noise-Conclusion
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This article is published in Bell System Technical Journal.The article was published on 1945-01-01 and is currently open access. It has received 807 citations till now.read more
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Strong chaos induced by close encounters with Ceres and Vesta
TL;DR: In this paper, the authors consider the full Solar System including the main asteroids and some of the smaller asteroids, and show that close encounters among these small bodies induce strong chaotic behavior in their orbits and in those of many asteroids that are much more chaotic than previously thought.
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Two-dimensional droplet spreading over random topographical substrates.
TL;DR: In this paper, the authors examined theoretically the effects of random topographical substrates on the motion of two-dimensional droplets via statistical approaches, by representing substrate families as stationary random functions.
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On the prediction of intermittent turbulent flows
TL;DR: In this article, a theoretical model is presented which permits the conservation equations of fluid dynamics to be conditioned in a fashion analogous to the experimentalist's technique of "conditioned sampling", which results in predictions of the flow variables within the turbulent flow and of the intermittency.
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Stabilization of optical phase/frequency of a laser system: application to a commercial dye laser with an external stabilizer
Miao Zhu,John L. Hall +1 more
TL;DR: In this article, the authors present a comprehensive and quasi-tutorial review of the theory for analyzing the optical power spectrum of an optical field that has noise modulations of both the amplitude and the phase.
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Shaken and stirred : the Milky Way's dark substructures.
Till Sawala,Pauli Pihajoki,Peter H. Johansson,Carlos S. Frenk,Julio F. Navarro,Kyle A. Oman,Simon D. M. White +6 more
TL;DR: In this article, the authors used the Apostle cosmological simulations to predict the abundance and the spatial and velocity distributions of subhaloes in the range 106.5-108.5m⊙ inside halos of mass ∼1012 m⊆ in Λ cold dark matter.